This galaxy exhibits a relatively smooth morphology, though some features are discernible. The light distribution is highly concentrated, suggesting a large spheroidal component. The shape appears largely round, with only a small deviation toward an elliptical form. There may be a faint disk or spiral structure visible in certain bands. No signs of ongoing major mergers or significant tidal disturbances are detected. The galaxy is relatively massive, suggesting a large population of stars. Low levels of star formation may be occurring within the galaxy.
