The galaxy appears as a relatively smooth object, exhibiting a centrally concentrated light profile. It displays a predominantly elliptical morphology, with an axis ratio suggesting a slight elongation rather than a perfect sphere. The core region is bright and potentially hosts an active galactic nucleus, as hinted by the bright core region. Evidence of disk or spiral structures are not readily apparent in the image. No major mergers or tidal features are visible, although subtle disturbances may be present. The galaxy exhibits a colour gradient, where the core exhibits a slightly bluer colour compared to the outer regions, indicating that star formation is concentrated within the core. Based on the colour, it likely consists of a population of older stars. The galaxy has a moderate redshift, suggesting it is at a significant cosmological distance.
