The galaxy presents as an elliptical morphology, generally smooth in appearance with a concentrated central bulge. There is little evidence of spiral arm structure or significant dust lanes. The color profile suggests an older stellar population, with light tending toward the redder end of the spectrum, especially within the central region. The galaxy has an intermediate axial ratio, appearing somewhat flattened but not highly elongated. There might be a slight asymmetry in the outer regions of the galaxy, suggesting a possible past interaction, though the bulk of the galaxy seems undisturbed. Overall, it presents as a relatively quiescent system, likely with low ongoing star formation.
