The galaxy appears to be a relatively smooth, elliptical galaxy, with a noticeable, bright central bulge. The light distribution suggests that the galaxy is mostly composed of older stellar populations, evidenced by the reddish-yellow hue and a lack of distinct blue regions typically associated with ongoing star formation. The overall shape is largely round. There may be a very slight asymmetry or minor disturbance in its morphology, but it is primarily a well-defined single structure without strong indications of a recent major merger or significant tidal interactions. Its color suggests it is not very actively forming new stars.
