The galaxy appears as a centrally concentrated, somewhat amorphous structure with a predominantly smooth morphology. There is evidence of a disk but it is difficult to distinguish it from its shape. Its overall color profile suggests a moderately evolved stellar population. The lack of distinct spiral arms, coupled with a generally homogenous appearance, indicates it is likely an early-type galaxy, such as an elliptical or lenticular. Subtle disturbances in the outer regions suggest potential minor gravitational interactions, possibly indicative of past or ongoing minor mergers or accretion events. The morphology can also be described as in between round and elliptical. There is no strong evidence of a major ongoing merger or significant tidal disruption.
