The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, centrally concentrated morphology. It is largely featureless with no discernible spiral arm structure or significant dust lanes visible in this imaging. The central bulge is prominent and roughly circular, with a radial decrease in surface brightness. The overall color appears relatively red, suggesting a population dominated by older stars and a low rate of ongoing star formation, although there may be some star formation occurring. The galaxy displays a degree of interaction or disturbance in its shape.
