This galaxy presents as a somewhat amorphous and centrally concentrated luminous object. The light is distributed in a fairly smooth manner, suggesting a lack of strong spiral arm structures or prominent dust lanes. The color appears generally yellowish-white, indicative of a stellar population that is neither dominated by young, hot blue stars nor extremely old, cool red stars. The overall shape tends toward round. There is a clear absence of any major tidal disturbances or obvious signs of interaction with other galaxies, though a possibility of an ongoing or past minor merger cannot be ruled out based on the image alone. The smoothness suggests that it could potentially be an elliptical or lenticular galaxy, rather than a spiral one. The overall impression is of a mature galaxy with moderate star formation activity.
