The galaxy appears as a faint, compact object with an overall smooth morphology. It presents a slightly elongated, disc-like structure with a relatively bright central bulge. There are faint hints of spiral arms, but these are not well-defined. The galaxy exhibits a color gradient, with the central region appearing more yellowish-white, potentially indicating an older stellar population or the presence of dust. The outer regions appear bluer, suggesting the presence of younger, hotter stars and ongoing star formation. There is no obvious evidence of a major merger event or significant tidal disturbances. The galaxy is well-resolved enough to distinguish these core features.
