The galaxy appears as a relatively smooth, elliptical-type object. It presents a centrally concentrated luminosity profile, with a bright core that gradually fades towards the outer regions. The galaxy exhibits a yellow-orange hue in its central region, suggestive of an older stellar population. There is little evidence of significant dust lanes or spiral arm structures. The overall shape is largely spheroidal, with a slight suggestion of ellipticity. No prominent tidal features or signs of recent major merger activity are readily apparent. The general morphology suggests that the galaxy is relatively undisturbed, likely in a late stage of its evolution.
