The galaxy presents an elongated morphology, appearing cigar-shaped. The primary structure exhibits a smooth light distribution, which indicates it is likely an elliptical galaxy. There is a hint of a possible disk or feature present, perhaps in the form of tidal debris. The color profile demonstrates a concentration of redder hues towards the central region, suggesting an older stellar population. Conversely, bluer colors are observed in the outer regions, which could potentially represent a more recent episode of star formation. The galaxy does not present any obvious signs of a major ongoing merger, but there are hints of minor disturbances that suggest a past or ongoing interaction with a smaller companion. The light is centrally condensed, though some diffuse light extends out from the main body of the galaxy.
