The galaxy presents as a system with a generally smooth morphology, though some subtle features are present. The central region displays a concentrated, bright core, suggesting a high stellar density. Surrounding the core is a more diffuse halo of light, exhibiting a gradual decrease in intensity with increasing radial distance.

The galaxy appears to be slightly elongated in shape. There is an indication of asymmetry or minor disturbance in the outer regions. A faint, irregular structure suggests potential tidal interactions or recent accretion events.

Color gradients are apparent, with the core exhibiting a yellowish hue, which may indicate the presence of an older stellar population. The outer regions show a bluer tinge. The overall color profile suggests a mix of stellar populations.
