The galaxy presents as an elliptical or lenticular system, with a smooth, largely featureless morphology. It appears highly centrally concentrated, lacking prominent spiral arms or distinct bar structures. The light profile shows a gradual decrease in intensity from the core to the outer regions. The galaxy's color is generally consistent, with a slightly bluer hue near the center transitioning to redder tones in the outer regions. This color gradient suggests older stellar populations in the outer regions. There are no visible signs of active galactic nuclei activity, significant dust lanes, or ongoing major mergers. The galaxy's rounded appearance indicates a relatively relaxed system that is close to equilibrium. Minor irregularities in the outer envelope may point to past minor interactions or tidal stripping events. The size of the galaxy is relatively small, suggesting it may be a dwarf or intermediate mass elliptical galaxy. The overall morphology suggests a relatively passive system, likely with limited ongoing star formation activity.
