The galaxy appears to be an elliptical or lenticular galaxy, displaying a smooth, centrally concentrated luminosity profile. It exhibits a subtle elongation, with the major axis extending roughly twice the length of the minor axis. There is a noticeable color gradient, transitioning from a yellowish-white core to a slightly redder halo. The lack of defined spiral arms or prominent dust lanes suggests a relatively quiescent state in terms of star formation. No evidence of major mergers or tidal disturbances are apparent in this observation. The light is distributed evenly throughout the galaxy body. The galaxy appears to have a very high concentration of old stars.
