The galaxy presents as an elliptical morphology, appearing largely smooth and featureless. The light profile exhibits a concentrated central bulge with a diffuse outer halo. There is evidence of color gradients, with the core of the galaxy exhibiting a yellowish-white hue, suggesting an older stellar population. A subtle reddish tint appears localized asymmetrically to the galaxy, potentially indicative of ongoing star formation, or dust lanes. The overall structure suggests a system that is likely evolved, with a dominant spheroidal component. There appears to be no significant tidal disturbance or signs of a recent major merger. The overall size suggests this is an average to large galaxy.
