The galaxy presents as a centrally concentrated spheroid with a smooth, diffuse profile. Its overall color appears to be a yellow-red hue, suggesting a relatively older stellar population. There is a notable lack of distinct spiral arm structure or prominent dust lanes. The observed ellipticity indicates a deviation from a perfectly circular shape, possibly due to intrinsic structure or viewing angle. No signs of recent or ongoing major mergers are apparent, though subtle asymmetries or minor disturbances cannot be completely ruled out based on this image alone. The general morphology suggests a classification leaning towards the elliptical or lenticular types. The estimated size is approximately 10 kpc in radius. Star formation appears to be quiescent.