The galaxy appears as a somewhat elliptical, smooth object with a concentrated central bulge. There is a subtle color gradient, with the central region exhibiting a yellowish-white hue, possibly indicating an older stellar population. The outer regions of the galaxy are less distinct and have a slightly bluer tint, hinting at the presence of some younger stars or possibly a very low level of ongoing star formation. The overall morphology suggests a relatively evolved system with minimal signs of recent major mergers or significant tidal disturbances. There is no clear spiral structure evident.
