The galaxy presents as a relatively small, faint object with a predominantly smooth morphology. The light distribution suggests a centrally concentrated structure, possibly a bulge, with a gradual decrease in intensity outwards. There is a hint of a disk-like structure but not a defined spiral arm or bar. A slight elongation is perceptible. Color gradients are subtle, but there appears to be bluer light concentrated in the central region that becomes slightly redder farther from the center. This could indicate older stellar populations in the outer regions. Overall, the galaxy's features suggest a classification leaning towards lenticular or possibly an early-type spiral galaxy seen at a low inclination. There is evidence that a merger may be occurring, perhaps with a minor disturbance or another merger.
