The galaxy presents as a moderately bright, elliptical-like object. It exhibits a smooth, centrally concentrated light profile, with the intensity decreasing gradually from the core outwards. The core appears to be a yellowish-white hue, potentially indicative of an older stellar population. A subtle disk is present with a slight tilt towards the upper right. The outer regions fade into a more diffuse, bluish halo, suggesting the presence of a younger stellar population or possibly some ongoing star formation. The galaxy's shape appears somewhat flattened, with the major axis oriented roughly horizontally in the image. There is no clear evidence of spiral arms or significant dust lanes within the observed wavelengths. Overall, the galaxy appears to be a relatively evolved system, likely dominated by older stars in the central regions.
