The galaxy presents a generally smooth morphology with a high degree of roundness. The central bulge is prominent and exhibits a yellowish-orange hue, indicative of an older stellar population. Fainter, slightly bluer regions are visible in what appears to be a diffuse disk surrounding the central bulge. There are subtle signs of tidal disturbance or merging activity, potentially in the form of faint plumes or asymmetries in the outer regions of the disk. The galaxy appears to be relatively isolated.
