The galaxy presents as a smooth, elliptical-like structure with a concentrated central bulge. The overall color profile appears to be yellowish-white, suggesting a population of older stars. The isophotes are generally regular, and the galaxy does not exhibit prominent spiral arms or significant dust lanes. There is minimal evidence of recent star formation activity. The galaxy appears relatively isolated, with no obvious signs of major tidal disturbances or ongoing mergers with other galaxies, though a very slight asymmetry hints at a possible minor interaction in the past. The galaxy is relatively compact, with a gradual decline in surface brightness from the core outward. 
