The galaxy presents a somewhat amorphous structure, lacking a well-defined spiral arm morphology or elliptical shape. It exhibits a central bulge, appearing yellowish-orange, possibly indicative of an older stellar population. Extending from the central bulge is a bluer, more diffuse region, suggesting the presence of younger, hotter stars and potential ongoing star formation. There is also a tidal tail extending from the galaxy, indicating potential ongoing merging. The overall light distribution seems relatively smooth, although subtle irregularities are present. The galaxy doesn't display a strong degree of rotational symmetry, implying it may be undergoing a disturbance or interaction.
