The galaxy presents an overall smooth morphology, suggestive of an elliptical or lenticular type. The light distribution appears centrally concentrated with a gradual decrease in intensity outwards. It is moderately elliptical in shape, with a slight elongation. The central region exhibits a brighter, more diffuse glow, possibly indicating a bulge component. There are no distinct spiral arms or prominent dust lanes visible. Faint color variations can be discerned across the galaxy's surface. A slight redder tint is visible in a small area, possibly indicating a region of older stellar populations or dust obscuration. Overall, the galaxy appears to be a relatively quiescent system with little evidence of ongoing star formation.
