The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, exhibiting a high degree of radial symmetry. The core region is characterized by a yellowish-white hue, suggestive of an older stellar population. The color gradually transitions to a bluer, albeit faint, outer halo. There is no strong visual evidence of spiral arm structure or significant dust lanes. Minor asymmetry might be present in the lower right quadrant of the halo. The light distribution suggests minimal ongoing star formation, with the bulk of the stellar mass concentrated in the spheroidal component. There is no sign of tidal disruption or a major merger event currently in progress, though subtle disturbances cannot be entirely ruled out.
