The galaxy presents a predominantly smooth morphology. It exhibits a centrally concentrated luminosity profile, with a bright, yellowish core gradually fading outwards. The overall shape approximates a flattened spheroid, leaning towards round rather than elongated. There are some subtle features, suggesting the possibility of a disk. The color distribution indicates a significant population of older stars, contributing to the yellow-red hue, but a bluer component is also present. There is no obvious evidence of a major ongoing merger, though subtle disturbances may be present in the outer regions, potentially indicating past interactions. The galaxy appears relatively isolated.
