The galaxy presents as a generally smooth, concentrated object with an apparent elongation. The primary body exhibits a bright central region that fades toward the periphery. The galaxy's overall color is skewed towards the redder wavelengths, with a noticeable yellow-orange hue dominating the central region. A less concentrated region is visible adjacent to the main galaxy. The smooth appearance suggests a relatively evolved stellar population, though the elongation hints at potential rotational dynamics or tidal interactions. There appears to be at least one neighbor to this galaxy. Further spectral analysis is recommended to confirm stellar population characteristics and internal dynamics.
