The galaxy presents as a somewhat elliptical, centrally concentrated object. The core exhibits a bright, yellowish-orange hue, indicative of an older stellar population. This central region gradually fades into a more diffuse halo. The outer regions display a subtle bluer tint and a slightly irregular shape. There is no discernible spiral structure or bar. Faint and subtle features suggest minor disturbances, possibly due to a past merger or ongoing interaction. The galaxy appears relatively smooth overall.
