The galaxy presents as a fairly smooth, elliptical-like structure. It exhibits a concentrated central bulge of moderate intensity, surrounded by a more diffuse halo. The light distribution appears relatively uniform, with no obvious spiral arms or distinct features. The color gradient suggests a higher concentration of older stellar populations in the core region, transitioning to bluer, potentially younger stars within the outer halo. There's a marginal suggestion of tidal disturbances or asymmetries, but the overall morphology leans towards a settled, spheroid-dominated system. Overall, the galaxy is most likely an elliptical galaxy, but further investigation into its stellar population and kinematic properties may be required.
