The galaxy presents a largely smooth morphology, suggestive of an elliptical or lenticular classification. The color distribution indicates a relatively older stellar population, concentrated towards the central regions. This is evidenced by the predominantly redder hues observed in the core, transitioning to slightly bluer tones towards the outer edges. The overall shape appears relatively round, with no distinct spiral arm structures or significant tidal disturbances visible. There is a slight indication of disk-like features, though they are not prominent. No signs of a major ongoing merger event are apparent. Overall, the galaxy seems to be in a relatively quiescent state, with a low rate of star formation.
