The galaxy presents as a slightly elongated, lenticular object with a smooth, diffuse light distribution. There is little evidence of spiral arm structure or significant dust lanes. The galaxy appears to be relatively isolated, with no obvious signs of ongoing major mergers or tidal interactions. Color gradients suggest a slightly bluer core region, potentially indicating recent or ongoing star formation. The outer regions exhibit a redder hue, consistent with an older stellar population. The overall morphology appears relatively undisturbed, indicative of a galaxy that has largely settled into a stable configuration.
