The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer regions. There is no strong evidence of spiral arms or a distinct disk structure. The galaxy appears slightly elongated, though not dramatically so. The color profile suggests an older stellar population, with a general lack of intense blue regions indicative of ongoing, massive star formation. There are hints of slight disturbances in its overall shape, however no clear merging event or strong tidal features are evident.
