The galaxy presents an overall elliptical morphology, appearing as a relatively smooth, centrally concentrated object. A notable feature is its subtle disk-like structure, exhibiting a slight flattening along one axis. The central region appears brighter and more uniform in color, trending toward a warmer hue. Fainter, bluer regions extend outward from the core, suggesting the presence of some star formation. The outer regions of the galaxy gradually fade into the background, with no prominent tidal features or significant morphological disturbances immediately apparent in this observation, though there may be some minor distortion of the disk. The galaxy exhibits an intermediate level of roundness, being neither perfectly spherical nor extremely elongated. The image suggests the galaxy is not currently undergoing a major merging event, but may have experienced minor interactions in the past that disturbed the structure.
