The galaxy presents as a fairly smooth, elliptical structure. Its central bulge is prominent and appears yellowish, likely indicating an older stellar population. Moving outward from the core, the light gradually diffuses into a fainter, less structured halo. There may be a hint of a disk component present, but it is not well-defined. There are no obvious signs of strong spiral arms, bars, or active star formation regions.

The galaxy appears relatively isolated, showing no major signs of tidal disruption that might suggest an ongoing or recent merger event. Minor asymmetry is noted, possibly caused by a past interaction or internal processes. Overall, the galaxy appears to be a relatively quiescent system dominated by older stars.
