The object presents as a single galaxy with a complex morphology, appearing to be in a state of interaction or recent merger. The primary component exhibits an elongated, elliptical shape with a smooth, diffuse light distribution characteristic of an elliptical galaxy or the bulge component of a spiral galaxy. This central region is dominated by a yellowish hue, suggesting a population of older stars.

Connected to this primary component is a secondary, distinct luminous region. This region displays a bluer color, potentially indicating a younger stellar population and ongoing star formation. This feature could be a tidal tail, a merging dwarf galaxy, or a region of intense star formation triggered by the interaction. There appear to be multiple regions of varying color and luminosity indicating a complex structure possibly due to an ongoing merger.
