The galaxy exhibits a somewhat elongated morphology. The central region displays a high concentration of light, appearing largely smooth and orange-yellow in color, suggesting an older stellar population. Extending from the core is a less defined, somewhat fainter, and bluer plume-like structure, possibly indicative of tidal debris or an ongoing interaction. This plume shows some irregularities and a slight curvature. The overall structure hints at a possible merging event or gravitational disturbance within the galaxy's recent history. Star formation may be occurring within the bluer regions.
