The galaxy presents an overall smooth, elliptical morphology, suggesting an older stellar population. Its shape appears moderately elongated, deviating somewhat from a perfect spheroid. There is a subtle hint of a disk-like structure, but it is not prominently defined. The galaxy's light is concentrated towards the center, diminishing gradually outwards. No spiral arms or significant dust lanes are readily apparent. There may be some minor distortions present, indicating possible past or ongoing interactions with another galaxy, or the remains of a small merger event. The colour suggests that the galaxy is actively forming stars. The galaxy appears relatively isolated, though with close inspection some interactions or tidal tails cannot be ruled out.
