The galaxy presents as a somewhat diffuse object, exhibiting a moderately elliptical morphology. There's a noticeable central bulge, characterized by a concentrated luminosity profile, transitioning smoothly outward into what appears to be a more extended halo. The overall color is consistent with an older stellar population, exhibiting a redder hue. There is a possible visual indication of a minor tidal disturbance or interaction with a smaller object nearby, which could contribute to the irregularity in the halo. Star formation appears subdued, with the dominant light emanating from evolved stars within the galaxy. The galaxy appears to be more lenticular than spiral, with some features to indicate a disk but without defined arms.
