This galaxy appears to be a lenticular or elliptical type. It exhibits a smooth, concentrated central bulge that dominates its overall structure. The light distribution shows a clear peak at the nucleus, gradually decreasing outwards. The galaxy presents an elongated, cigar-like shape, indicating a significant ellipticity. There is a lack of distinct spiral arm features, which suggests a relatively quiescent star formation history. No signs of strong tidal disturbances or ongoing major mergers are readily apparent from the image. The galaxy is largely a homogenous color, primarily white, indicative of a relatively older stellar population with a low ongoing rate of star formation.
