The galaxy presents as a compact, elliptical-like structure. It has a predominantly smooth appearance, with no apparent spiral arms or significant dust lanes visible. The galaxy's light profile appears relatively concentrated towards the center, suggesting an older stellar population is dominant. There is a slight elongation or deviation from perfect roundness. The color appears to be relatively uniform across the galaxy, leaning toward the redder end of the spectrum, indicating the presence of older, redder stars and a lack of significant ongoing star formation. There does not appear to be any evidence of tidal tails or other obvious signs of recent or ongoing mergers.
