The galaxy exhibits a generally smooth morphology. It appears largely spheroidal in shape, with a high degree of central concentration of light. The color profile suggests a predominantly older stellar population, with a yellowish core indicative of evolved stars. The outer regions show a slightly bluer tint, suggesting the presence of some younger stars or ongoing, though limited, star formation. There is no obvious spiral structure or pronounced disk component. The galaxy appears relatively undisturbed, with no significant signs of tidal interactions or recent major mergers. A slight asymmetry in the outer isophotes hints at a possible minor interaction. Overall, this galaxy presents as a relatively massive, evolved system, potentially an elliptical or an S0 galaxy.
