The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. The color profile is generally redder, with a slight gradient towards bluer hues in the outer regions. There is no clear evidence of spiral arm structure or significant dust lanes. The overall morphology suggests a more evolved system. The light distribution appears centrally concentrated, indicative of a possible spheroidal galaxy type. There does not appear to be any major merger events or tidal disturbances affecting the galaxy's structure. A minor asymmetry may be present in the outer regions.
