The galaxy presents as a centrally concentrated, elliptical structure with a smooth light distribution. The core is a bright, yellowish-orange hue, indicating a population of older stars. There is a subtle color gradient extending outwards from the core, transitioning to a redder tone, which suggests the presence of a somewhat older stellar population towards the galaxy's periphery. No distinct spiral arms or dust lanes are discernible. The general morphology suggests a relatively evolved system, possibly an elliptical galaxy undergoing passive evolution. Faint, diffuse emission is observed surrounding the galaxy, hinting at a tenuous halo or extended stellar component. There is no strong evidence of ongoing star formation.
