The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth light distribution. There is a distinct lack of defined spiral arms or prominent dust lanes. The color profile appears generally red-shifted, suggestive of an older stellar population and relatively low levels of ongoing star formation. The galaxy's shape exhibits a degree of elongation, deviating from a perfectly circular form; instead, it shows a more cigar-like appearance. No signs of significant tidal disturbances, close companion galaxies, or any other morphological peculiarities that would indicate a major recent merger are obviously visible. There are hints of blue-ish light on the very edges of the galaxy, suggestive of possible faint star formation. 
