The galaxy presents as an elliptical morphology, appearing mostly smooth with a bright, concentrated central bulge. The light distribution seems fairly uniform, lacking any distinct spiral arm structures or prominent dust lanes. Color gradients are subtle, with a yellowish core gradually transitioning to a bluer halo. Overall, the galaxy exhibits features consistent with an older stellar population and subdued star formation activity. There is a possible slight elongation or tidal disturbance in the morphology, potentially hinting at past or ongoing interactions with other galaxies, but it does not seem to be undergoing a major merger.
