The galaxy presents a generally smooth morphology, with a centrally concentrated luminosity profile. The shape appears neither perfectly circular nor highly elongated, exhibiting an intermediate ellipticity. There is evidence of some internal structure, possibly indicative of a disk component or spiral arms, though these features are not sharply defined. The galaxy displays a color gradient, with the central region appearing more yellow/orange, potentially indicative of an older stellar population or significant dust extinction. The outer regions appear bluer, suggesting younger stars or less dust. There are no obvious signs of major mergers or tidal disturbances, although subtle asymmetries may hint at past interactions. The galaxy's estimated size suggests it is a moderate sized object. Star formation appears to be ongoing, but is at a modest rate. Overall, the galaxy appears to be an intermediate mass system, possibly undergoing a transition in its star formation history.
