This galaxy appears to be a relatively smooth, elliptical-type galaxy. The central bulge is prominent and exhibits a bright, concentrated luminosity gradient. Moving outward from the core, the light gradually fades into a less defined halo. There is a slight elongation of the galaxy, appearing as an in-between rounded shape rather than a perfectly circular distribution of light. The galaxy exhibits a blue hue and a moderate color gradient from the center outwards, suggesting some ongoing star formation, though not intensely active. There are some minor disturbances likely from a small merger event. Overall, it appears to be a somewhat massive galaxy with intermediate star forming activity.