The galaxy presents as a single, concentrated body with a centrally-peaked light profile indicative of a substantial bulge component. The galaxy exhibits a smooth, elliptical morphology with a generally round shape; there is no evidence of spiral arms or a distinct disk structure. The light distribution is somewhat diffuse towards the outer edges, gradually fading into the background. There are no prominent features suggestive of recent major merger activity or tidal disturbances; any merger events were likely minor. The galaxy displays a yellow-orange hue, suggesting an older stellar population and relatively low current star formation. The central region appears brighter and more concentrated than the surrounding area, which is likely to host an accreting supermassive black hole.