The galaxy presents a predominantly smooth morphology, with minimal discernible features indicative of spiral arms or a prominent disk structure. It appears relatively compact with a moderate degree of roundness, although it does not present as perfectly spherical. There is a subtle color gradient observed, transitioning from slightly bluer hues in the central regions to redder tones in the outer regions, possibly suggestive of an older stellar population in the outskirts. There is no obvious evidence of ongoing major mergers or significant tidal disturbances impacting the galaxy's structure. Faint color variations could be indicative of some recent or low-level star formation activity. Overall, the galaxy appears consistent with an elliptical or lenticular galaxy.
