The galaxy presents an overall elliptical morphology, with an approximate semi-major axis extending further than the semi-minor axis. The light profile is smooth and centrally concentrated, exhibiting a gradient in color. The core of the galaxy appears more yellow and red compared to its outer regions, with a transition towards bluer tones as one moves outward from the nucleus. This suggests a population of older stars and possibly dust obscuration near the center, with younger stars and less dust in the periphery. While the main body of the galaxy shows a largely undisturbed structure, there are subtle irregularities suggesting possible minor interactions or internal dynamics that are causing very slight disturbances to its otherwise smooth form. There is no evidence of strong tidal features, but a very faint and small extension can be noted in its morphology.
