The galaxy presents as a fairly smooth, elliptical or lenticular type, with an apparent cigar shape along its major axis. The central bulge exhibits a concentrated, bright, yellowish-white hue, suggesting a relatively older stellar population. The galaxy's overall color is slightly redder than the central bulge. There's a subtle hint of a disk component, though it's not particularly prominent. There is no strong evidence of spiral arm structure or significant dust lanes. There are no indications of ongoing major mergers or significant tidal disturbances.
