The galaxy presents an overall smooth morphology with a slight elongation in its shape. The light distribution appears centrally concentrated, suggesting a dominant bulge component. The color profile indicates an older stellar population dominating the galaxy's composition, with a redder hue concentrated in the central region and a subtle bluer tint extending outwards, hinting at possible ongoing star formation in the outer regions, though at a low rate. There is a potential faint tidal feature or minor disturbance on one side of the galaxy, suggesting a possible past interaction or merger event. Overall, the galaxy appears to be an intermediate mass system, likely undergoing a slow process of quiescence.
