The galaxy presents an overall elliptical morphology, with a relatively smooth light distribution. The object appears largely spheroidal, with a degree of elongation, suggesting a possible classification between E3 and E5 on the Hubble sequence. The color is relatively uniform across the galaxy, with the central region appearing slightly more yellow/orange than the outer regions. This could indicate a higher concentration of older stars towards the core. There is evidence of a slight tidal disturbance, with some faint wisps or extended features. The galaxy could be undergoing minor interactions. The light profile appears relatively concentrated.
