The galaxy presents as an elliptical morphology, with a smooth light distribution and no distinct spiral arm structure visible. The central bulge region appears bright and concentrated, characterized by a yellow hue suggestive of an older stellar population. Moving outwards from the core, the light gradually fades into the surrounding halo, which possesses a reddish tinge. The relatively smooth texture with no distinct dust lanes or prominent star-forming regions suggests a relatively low ongoing star formation rate. The galaxy is relatively isolated, without apparent signs of tidal interactions or nearby companions, and the overall shape is neither perfectly spherical nor elongated.
