The galaxy exhibits a generally smooth morphology, with a high degree of roundness. There is little indication of spiral arm structures or other distinct features typically associated with disk galaxies. The galaxy appears largely undisturbed, showing no signs of major mergers or significant tidal distortions. A slight asymmetry may be present, suggesting possible minor gravitational interactions or internal activity. Based on the color profile, the galaxy is likely comprised of an older stellar population, with potentially low ongoing star formation. The estimated size of the galaxy suggests that it is a moderate-sized system.
