The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal. A central bulge dominates the structure, exhibiting a concentrated intensity of reddish hues. This color suggests a population of older, redder stars, indicative of a relatively quiescent star formation history within the bulge. Surrounding the bulge is a broader, less intensely colored halo. This halo exhibits a greenish tint, potentially indicating the presence of a younger stellar population or some ongoing star formation, though at a seemingly low rate. There's little evidence of spiral arms or significant dust lanes, reinforcing its classification as an elliptical galaxy. The galaxy is relatively isolated, showing no obvious signs of recent mergers or tidal interactions with neighboring galaxies.
