The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth and centralized luminosity profile. The central region is characterized by a bright, concentrated core which fades gradually into the surrounding halo. There's a subtle color gradient visible, with the core tending towards yellower hues, suggesting an older stellar population, and the outer regions appearing slightly bluer, possibly indicating the presence of some younger stars or regions of limited star formation. No distinct spiral arms or bar structures are discernible. Overall, the galaxy appears relatively undisturbed, showing no strong signs of ongoing mergers or significant tidal interactions. Subtle irregularities are observed, but no features indicating major disturbances.
