The galaxy presents an elliptical morphology, appearing mostly smooth with a slight elongation. Its color profile indicates a significant population of older stars, with a dominant yellowish hue in the central bulge. There's little evidence of active star formation. It exhibits a relatively high degree of central concentration, with luminosity decreasing gradually from the core outwards. No prominent spiral arms or distinct dust lanes are discernible, and there is no strong evidence of any ongoing major merger activity or significant tidal disturbances affecting the galaxy's structure. The overall structure suggests it is a relatively quiescent galaxy.