The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The color is generally yellowish-orange, suggestive of an older stellar population. No distinct spiral arm structure or dust lanes are visible. The galaxy appears fairly isolated, showing no strong signs of tidal distortion or ongoing mergers, though there may be some minor disturbances within the halo. The overall roundness indicates a low degree of flattening. The estimated size is relatively small for a galaxy, with the light being concentrated to the core. Star formation is likely suppressed, as inferred by the color and lack of prominent features associated with active star formation.
