The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated central bulge. It exhibits a slightly elongated, but generally rounded morphology. There is little evidence of distinct spiral arms or significant dust lanes. The color gradient suggests an older stellar population, with a yellowish-white core indicating a concentration of older stars. The outer regions of the galaxy fade into the background with a slightly bluer tint, which may indicate some ongoing low-level star formation, but predominantly this is an older stellar population with an estimated stellar mass slightly more than 10^9 solar masses. The overall smooth structure suggests that it is not currently undergoing a major merging event, although there may be some minor gravitational disturbances present in the outer regions.
