The galaxy appears to be a relatively smooth, elliptical structure. It exhibits a bright, concentrated central bulge, which gradually diffuses outward into a fainter, more extended halo. The overall color is yellowish-orange, suggesting a population of older stars and a relatively low rate of ongoing star formation. There is no visible evidence of spiral arms or significant dust lanes. The galaxy's shape is moderately elongated, appearing more like a flattened spheroid than a perfect sphere, which is characteristic of E3-E5 galaxies. There are no visible signs of tidal tails or other distortions indicative of a recent merger event, though subtle disturbances cannot be ruled out at this resolution. The galaxy seems relatively isolated within the observed field, with no other nearby objects appearing to significantly interact with it.
