The galaxy presents a generally smooth appearance with a slight flattening. The central region exhibits a high degree of luminosity, characterized by a bright, concentrated core that fades gradually outwards. There appears to be some structure, such as a disk, as it has some asymmetrical features. Overall, the color profile appears to be largely homogenous, with a subtle shift toward redder hues. A low star formation rate is likely present. No strong signs of ongoing mergers or interactions are apparent in the visible light.
