The galaxy presents as an elliptical or lenticular system, elongated in shape with a smooth, concentrated central bulge. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population. The overall color gradient transitions towards a slightly bluer shade in what could be a very faint and diffuse disk surrounding the bulge. There is a slight asymmetry in brightness between the top and bottom halves of the galaxy, with a fainter extension on the bottom side, possibly indicative of minor tidal interactions or past mergers, but could also be a star forming region. There appears to be no prominent spiral arm structure, or significant dust lanes are visible in this particular image, indicating a lack of ongoing major star formation. The galaxy appears relatively undisturbed in its overall morphology.
