The galaxy presents a largely smooth, elliptical morphology. It is highly concentrated with a bright central region that diffuses outwards. The overall shape is primarily round with a slight deviation towards a more elongated form. There is no clear evidence of spiral arm structure or a prominent disk. Faint hints of disturbances or minor irregularities are present in the outer regions, but the galaxy appears to be generally undisturbed, showing no signs of a major ongoing merger. The galaxy exhibits a redder hue, suggesting a population of older stars, with moderate ongoing star formation.
