The galaxy presents as a somewhat elongated, elliptical structure. A central bulge dominates the light profile. The core region exhibits a reddish-orange hue, which may indicate an older stellar population. There is a subtle transition to a greenish halo surrounding the central region, possibly indicating younger stars or ionized gas. The galaxy appears relatively smooth with no prominent dust lanes or spiral arm structures visible. The galaxy shows no signs of tidal disturbance or recent merger activity. Overall the galaxy appears to be a relatively isolated elliptical galaxy with ongoing, albeit low, star formation.
