The galaxy exhibits a morphology characterized by a centrally concentrated, luminous region, likely the bulge or core. This central region demonstrates a relatively smooth appearance with a bright, compact distribution of light.

Extending from this central concentration are fainter, diffuse features. One appears as a wispy arm or tidal tail, slightly curved and possessing a yellowish hue, suggesting an older stellar population or dust obscuration. Another separate feature shows a similar diffuse appearance, and bluer colour.

The overall shape could be described as disturbed or irregular, suggesting a possible interaction or merger event. There appears to be some deviation from a perfect elliptical or disk-like structure. A distortion can be seen in the lower part of the galaxy.
