The galaxy presents as a somewhat diffuse, centrally concentrated object. It exhibits a general yellowish-white hue, suggesting an older stellar population. The morphology appears relatively smooth with some minor features present. There does not appear to be a distinct, well-defined spiral arm structure or a prominent bar. The galaxy's overall shape appears to be generally elliptical. There are no clear signs of ongoing major merger activity or significant tidal disturbances. A slight asymmetry is present.
