The galaxy presents an overall smooth, elliptical morphology. It displays a centrally concentrated luminosity profile, suggesting a prominent bulge. The galactic structure shows a degree of elongation, deviating noticeably from a perfectly circular shape. The color profile indicates a population of older stars, with redder hues concentrated within the galactic core, and bluer hues visible toward its outer regions. There is evidence of some structural disturbance or tidal interaction, based on asymmetries in its outer isophotes, indicative of possible merging. Based on color, the galaxy is actively forming stars at a relatively slow rate. There is an absence of bright star-forming regions, also indicating a relatively quiescent star formation history and suggesting it is on the red sequence. The galaxy's estimated size is several kpc. Overall, the galaxy appears to be an elliptical galaxy undergoing some disturbance.
