The galaxy presents as a moderately luminous, ellipsoidal structure. Its overall color profile indicates a dominant population of older stars, evidenced by the redder hue. The light distribution is relatively smooth, with a highly concentrated central bulge that transitions gradually into an extended, less dense halo. There is no obvious spiral arm structure or dust lane obscuration visible. The overall morphology suggests the galaxy is an early-type, possibly an elliptical galaxy, showing a significant degree of sphericity. There appears to be a slight disturbance to the even symmetry.
