The galaxy presents as an elliptical morphology, with a smooth and concentrated central bulge. The light profile appears relatively uniform, lacking distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a subtle color gradient, transitioning from a yellowish-white core to a slightly redder halo. This suggests a population of older stars dominating the central region, with a possible presence of younger, bluer stars towards the outskirts. There appears to be a slight asymmetry to the overall shape, though it is subtle. No evidence of ongoing major merging activity or significant tidal disturbances is apparent, though a minor interaction cannot be ruled out due to the slight asymmetry. Overall the galaxy appears to be a fairly massive system with low star formation.
