The galaxy appears as an elliptical structure with a relatively smooth light distribution. The central region exhibits a higher surface brightness, gradually decreasing outwards. A slight elongation is visible, though the overall shape is mostly spheroidal. The colour profile suggests a population of older stars, with a dominant reddish hue. There are very faint hints of what could be minor disturbances in the outer regions, potentially indicative of past interactions or mergers. The galaxy lacks any prominent spiral arms or distinct features characteristic of younger stellar populations. Overall, the galaxy presents as a massive system consistent with a large elliptical morphology and a moderate degree of star formation.
