The galaxy presents a predominantly smooth, elliptical morphology with a bright, concentrated central bulge. There is a subtle elongation, tending towards an in-between roundness. No distinct spiral arms or bar structures are discernible. The color profile indicates a generally older stellar population with a yellowish hue in the central region, transitioning to slightly bluer tones in the outer regions, suggesting some ongoing star formation. No signs of major mergers or significant tidal disturbances are apparent, although there may be minor asymmetries. The galaxy appears to be relatively isolated. Overall, the galaxy seems to be a massive, evolved system.
