The galaxy presents as a somewhat amorphous structure, with a generally rounded morphology although some irregularities are visible. The central region appears relatively smooth and concentrated, exhibiting a yellowish-orange hue, suggesting an older stellar population dominates the core. Fainter, diffuse blue regions are sparsely distributed outside the core, indicating regions of ongoing, albeit potentially low-level, star formation.

There's evidence of possible tidal disturbances or interactions, suggested by the subtle asymmetries in the outer regions. The overall color profile indicates a mix of stellar populations, with a central bulge seemingly more evolved and quiescent compared to the bluer, potentially star-forming regions scattered within the galaxy’s disk. The presence of redder elements within the galaxy could also indicate the presence of dust obscuring some areas or further evidence of an older stellar population. The galaxy does not appear to have a distinct spiral or bar structure within the limits of this image.
