The galaxy presents as a flattened, elliptical structure. Its core region displays a concentrated, yellowish-white hue, suggesting an older stellar population. The outer regions exhibit a bluer tint, hinting at the presence of younger stars or ongoing star formation, though at a relatively low rate. The galaxy's overall form is elongated, with a slight distortion visible on one side, possibly indicating a minor gravitational interaction. Its morphology is primarily smooth, with hints of internal structure, potentially a faint disk component. There is no strong evidence of a major merger event, although a minor disturbance may be present. The color gradient from the core to the outer regions indicates varying stellar populations.
