The galaxy presents as a relatively smooth, elliptical-like structure. A bright, concentrated central bulge dominates the overall luminosity, with the light appearing to decrease gradually outwards. There is a slight elongation to the galaxy's shape, suggesting a deviation from perfect circularity, though it does not appear as a highly elongated spindle. No distinct spiral arm structures or prominent dust lanes are visible. The overall color appears relatively uniform, with a slight trend towards redder hues, indicative of an older stellar population and reduced star formation activity. There are no visually apparent signs of major mergers or significant tidal disturbances, although subtle asymmetries or minor disturbances cannot be entirely ruled out given the resolution. The galaxy appears relatively isolated within its immediate vicinity, with no obvious companion galaxies or significant interactions underway.
