The galaxy presents as a relatively compact object. Its overall morphology appears largely smooth and spheroidal. There is a noticeable color gradient, with a central region exhibiting a yellower hue, possibly indicating an older stellar population or a higher concentration of dust. The outer regions transition to a bluer tint, potentially suggesting the presence of younger, hotter stars or ongoing star formation activity in these areas, although this activity is not visually prominent. No spiral arm structure or significant dust lanes are discernible. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions.
