The galaxy presents as an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The core region displays a yellowish hue, possibly indicative of an older stellar population. Extending outwards from the core, the galaxy exhibits a diffuse, fainter halo with a bluish tint, perhaps signifying the presence of younger, bluer stars or ongoing star formation, albeit at a low rate. The object appears mostly undisturbed, displaying no signs of major mergers or tidal interactions. There is slight asymmetry present, possibly indicative of a minor interaction or internal structure within the galaxy. Overall, the galaxy appears to be a moderately massive system with a low specific star formation rate.
