The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. It presents with a concentrated central bulge that graduates outward into a diffuse halo. The color profile suggests a higher concentration of older stellar populations, indicated by a yellowish hue in the central regions. There is little evidence of distinct spiral arms or significant dust lanes. Overall, the galaxy seems to be relatively undisturbed with no apparent signs of ongoing major mergers or tidal distortions. A minor asymmetry is possibly detected in the galaxy's extended halo.