The galaxy presents as a somewhat symmetrical, diffuse object, exhibiting a centrally concentrated luminosity profile. The core region is bright and well-defined, showing a distinct white-blue hue, suggesting a potentially older stellar population or strong continuum emission. This central area is surrounded by a fainter, more extended halo or disk-like structure. The galaxy appears relatively smooth in texture with subtle irregularities. There is limited evidence of strong spiral arm structure or distinct dust lanes, the bluer color also suggests lower dust content. Overall, the galaxy displays characteristics consistent with an elliptical or lenticular morphology, possibly undergoing some minor interaction or disturbance.
