The galaxy presents as a largely featureless, elliptical morphology. The light profile is concentrated towards the center, indicating a significant central bulge. It appears as a smooth object, with no obvious spiral arm structure or dust lanes. The shape is elongated, tending towards a cigar-like appearance. The color gradient suggests a population of older stars, potentially with ongoing, low levels of star formation. There is no indication of a major merger event, though minor disturbances cannot be ruled out.
