The galaxy presents as an elliptical morphology, appearing largely featureless and smooth in texture. The galaxy exhibits a radial concentration of luminosity, with a bright, dense core that gradually fades towards the outer regions. Color gradients suggest a possible change in stellar population with radius, as the core appears more yellow, potentially indicating an older, redder stellar population, while the outer regions may have a slightly bluer hue. There is no evidence of spiral arm structures or significant dust lanes. The shape is close to circular, with a small deviation toward a cigar shape. No indications of major mergers or significant tidal disturbances are apparent; it seems to be a relatively isolated system in its current state.
