The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, grading outward into a more diffuse halo. The color profile suggests a population of older stars, indicated by its overall reddish-yellow hue. No distinct spiral arms or prominent dust lanes are discernible. The shape approximates a rounded form, though with a slight elongation. No significant tidal features or indications of recent major mergers are evident, implying a gravitationally settled state. There is a possibility of some minor disturbance in the galaxy due to a slight asymmetry and non-uniform light distribution in the halo. The galaxy appears to be undergoing minimal star formation.
