The galaxy presents a largely smooth morphology with a centrally concentrated luminosity profile. It exhibits a nearly elliptical shape, appearing only subtly elongated. No distinct spiral arm structures or bar features are discernible. The core region is bright and diffuse, gradually fading into the surrounding halo. There is no obvious indication of tidal streams or interaction with neighboring galaxies. The overall color appears relatively homogenous, with a slight shift towards redder hues compared to bluer ones. No distinct dust lanes or regions of active star formation are readily apparent in this image. The galaxy appears to be a mature system, with a lack of significant morphological disturbances.
