The galaxy presents as a relatively smooth, centralized structure. Its morphology appears largely elliptical, with a discernible elongation along one axis, giving it a slightly cigar-shaped appearance. The light distribution is centrally concentrated with a bright core, indicative of a possible supermassive black hole. There is a gradual decline in luminosity moving outwards from the core, with no distinct spiral arm features readily visible. Faint, diffuse light extends from the central region. There is no evidence of active galactic nuclei activity visible within the image. The galaxy color appears to be on the redder side, suggestive of an older stellar population, and low star formation rates. No signs of recent or ongoing merger events are apparent within the immediate vicinity of the galaxy.
