The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears bright and is a yellowish-orange hue, which likely indicates an older stellar population dominating the core. The galaxy's overall shape leans towards being in between round and elliptical, with a slight elongation visible. There are no readily apparent spiral arms or significant dust lanes interrupting the smoothness of the light distribution, suggesting it is primarily composed of older stars. There is no signs of a recent merger event, though there are minor disturbances. The galaxy appears to be at an intermediate redshift.