The object presents as a relatively compact galaxy with a notable central bulge. The overall color profile suggests a population of intermediate-age stars, as evidenced by the prominent yellow-green hue surrounding the core. There appears to be a degree of tidal distortion or minor interaction with a satellite galaxy, indicated by the slight irregularity in its outer isophotes. The color distribution is relatively uniform across the visible extent of the galaxy, with minimal indication of significant dust lanes or recent star formation. The shape of the galaxy is somewhat elliptical, with an estimated effective radius on the order of several kiloparsecs. No spiral arm structure is apparent from the image.
