The galaxy presents a generally smooth and rounded morphology. The central region appears to be dominated by an elliptical-like structure with a concentrated, bright nucleus. The color suggests a population of older stars, potentially indicating reduced star formation in the core. Surrounding the central region, a fainter, more diffuse halo is visible, exhibiting a slight bluish tint. This could be indicative of a population of younger, hotter stars, although star formation is not particularly active. There is no evidence of strong spiral arm structures or significant disturbances in the overall shape, such as tidal tails or merging features.
