The galaxy presents a largely smooth morphology, exhibiting an elliptical-like shape in this image. The light distribution is generally centrally concentrated with a bright core that fades gradually outwards. There is a slight elongation visible, however, it appears largely round. I observe a hint of a potential tidal feature or a minor interaction on its periphery. The galaxy appears to be relatively isolated, showing no strong signs of a major merger event in its recent past, though a weak disturbance cannot be ruled out. The colour index suggests the stellar population is comprised of older stars with little ongoing star formation.
