The galaxy presents a largely featureless appearance, with a smooth, elliptical morphology dominating the light profile. The core region exhibits a concentrated luminosity, appearing bright and yellowish-orange in color. Moving outward from the central region, the galaxy's light gradually diminishes, lacking any distinct spiral arm structures or prominent dust lanes. There might be a faint, diffuse disk present, though its contribution to the overall structure is minimal. The round shape of the galaxy is evident and there is no sign of significant disturbance or ongoing merger events. The overall color suggests a population of older stars, implying that the rate of current star formation is relatively subdued within the galaxy. The lack of prominent blue colors reinforces this observation.
