The galaxy presents a generally smooth, elliptical morphology. Its color index suggests it is likely an early-type galaxy with a dominant population of older stars. The galaxy appears somewhat round, lacking a strong disk-like structure or significant spiral arms. There is no obvious indication of a major ongoing merger or significant tidal disturbances in this particular image, though there are hints of minor structural variation. The size is relatively compact, indicating a possibly moderate physical extent. Star formation is suspected to be very low.
