The galaxy presents as an elliptical morphology, with a smooth, diffuse light profile. The central region exhibits a higher surface brightness, appearing more concentrated than the outer regions. There is a slight elongation observed in the galaxy's shape, tending toward a cigar-like form. Color gradients are subtle, with a suggestion of a bluer hue in the outer regions compared to the more yellow-toned central bulge. No distinct spiral arms or significant dust lanes are discernible. There does not appear to be any evidence of major ongoing merger activity or significant tidal disturbance in this image. The overall appearance suggests a relatively evolved system with a stellar population dominated by older stars, with low levels of ongoing star formation activity.
