The galaxy presents a predominantly smooth morphology with a concentrated central bulge. It appears elliptical in shape, exhibiting a slight elongation rather than a perfectly circular form. The galaxy's color profile indicates an older stellar population, with a yellowish hue dominating the central region. The outer regions transition to a redder tone, suggesting a decrease in younger, bluer stars and ongoing or recent star formation. No distinct spiral arms or bar structures are readily apparent. There is no immediately obvious evidence of major mergers or significant tidal disturbances affecting the system's overall structure, although some minor asymmetries might be present upon closer inspection. The light is centrally condensed but diffused in the outer edges. Overall, the galaxy gives the impression of a mature, relatively quiescent system.
