The galaxy appears as a centrally concentrated elliptical or lenticular system. It exhibits a smooth, luminous profile, with a dominant central bulge. The color gradient suggests an older stellar population, displaying a yellowish hue indicative of evolved stars. There is little evidence of prominent spiral arms or active star-forming regions within the main body. A slight asymmetry is visible in the outer regions, potentially indicating a minor disturbance or past interaction. The overall structure suggests a relatively quiescent galaxy, likely experiencing low rates of star formation. The estimated size indicates a substantial galactic mass.