The galaxy presents an overall reddish hue with a moderate degree of central concentration. The light distribution suggests a smooth morphology, potentially resembling an elliptical galaxy. However, there are subtle irregularities in the galaxy's outer regions. There is a hint of a disk-like structure, possibly a faint, diffuse spiral arm. The presence of these features suggests the possibility of a minor gravitational disturbance or tidal interaction with a nearby object. A slight asymmetry in the isophotes could further support this hypothesis. There does not appear to be an obvious presence of any major merging events.
