The observed galaxy presents a complex morphology, exhibiting both smooth and featured components. The central region appears relatively smooth, with a diffuse, somewhat elongated shape. There is evidence of asymmetrical structure suggesting it is not a perfect spheroid.

Extending outward from the main body of the galaxy, a fainter, extended component is visible. The outer regions display irregular features, with suggestions of tidal debris or disrupted structures. Faint wisps of material appear to be stretched and distorted, potentially indicating gravitational interactions with another galaxy. The colour gradient shifts noticeably, possibly indicative of varying stellar populations or dust extinction along this feature.

There are faint indications of potential minor disturbances within the galaxy's structure, though more data would be needed to accurately describe any interactions.
