The galaxy presents a somewhat elongated, cigar-like morphology. It exhibits a smooth appearance, with approximately equal likelihoods of appearing purely smooth or demonstrating disk-like or featured characteristics. The color profile suggests a redder core, possibly indicative of an older stellar population, with bluer hues extending outwards, potentially indicating regions of more recent star formation. There is a notable absence of significant dust lanes or intricate spiral arm structures visible in this image, potentially due to limitations of image resolution, or could imply a more quiescent galaxy with minimal ongoing star formation. The overall light distribution is relatively even, suggesting a well-mixed stellar population and a lack of intense, localized star-forming regions. The galaxy does not appear to be currently undergoing a major merger, with the galaxy more likely to be isolated or only experiencing minor gravitational disturbances. The physical size is relatively modest, and estimated mass indicates a dwarf galaxy system. The inferred star formation rate is quite low, suggesting a very old stellar population.
