The galaxy presents a generally smooth and centrally concentrated morphology. The light distribution suggests a spheroid-dominated system, likely an elliptical or S0 galaxy. There's a slight elongation, but the overall shape is mostly round with a slight tilt. There is a central bright region, possibly indicating an active galactic nucleus or a dense stellar population. Fainter extended halo is present, particularly prominent in the blue light. Very little evidence of spiral arms or significant dust lanes. There appears to be some potential disturbance in the outer regions, suggesting minor past interactions. The overall color gradient indicates a significant population of evolved stars, with a possible indication of some ongoing, though not dominant, star formation.