This galaxy appears to be a relatively smooth, elliptical galaxy. There is no clear evidence of spiral arm structure or a distinct disk. The color profile suggests an older stellar population, with a general lack of blue light indicative of ongoing, rapid star formation, although some star formation is still likely present. The galaxy exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness moving outwards from the core. There is no obvious evidence of a major merger event or significant tidal disturbances in the immediate vicinity of the galaxy. The shape is approximately in between round and elliptical. There may be a very minor disturbance present.
