The galaxy presents as a relatively smooth, luminous object, with a slightly elongated morphology. It exhibits a centrally concentrated light profile, indicative of a possible bulge component. There are no obvious spiral arm structures or prominent dust lanes visible. The color appears to be moderately red, suggesting a population of older stars. A mild disturbance is indicated, there might be a faint tidal tail or distorted morphology, suggesting a possible interaction or merger event in its past. The galaxy is classified as intermediate in terms of roundness, not quite circular but not extremely elongated. Overall, the galaxy appears to be a relatively massive, evolved system with a modest level of recent star formation.
