The galaxy presents as a relatively compact object. Its overall shape is somewhat elliptical, appearing more rounded than elongated. The light distribution is mostly smooth, indicating a lack of significant spiral arm structure or prominent dust lanes. A subtle color gradient is observed, transitioning from a slightly bluer hue towards one end to a yellower, possibly redder, color towards the opposite end. This suggests a potential variation in stellar populations across the galaxy, with the bluer region possibly indicating more recent star formation activity, and the yellower/redder area being home to an older stellar population. Signs of disturbance are present, indicating the possibility of minor ongoing interactions or a past merger event.
