The galaxy presents a generally elliptical morphology, with a smooth, diffuse light distribution. The core region appears concentrated and exhibits a yellowish hue, suggesting an older stellar population. The outer regions show a bluer tint, possibly indicating a more recent episode of star formation, albeit at a low rate. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's overall structure suggests that it is an early-type galaxy transitioning from a more active star-forming phase. There are no obvious signs of tidal disturbances or interactions with other galaxies.
