The galaxy presents as a relatively compact object, appearing largely spheroidal in overall morphology. A prominent central bulge dominates the structure, exhibiting a yellowish-white hue, indicative of an older stellar population. There is asymmetry in the disk region. The brighter disk portion displays a gradual shift toward redder wavelengths, possibly due to the presence of dust obscuration or aging stellar populations within that segment. Indications of a minor tidal disturbance, possibly resulting from a recent interaction or merger.
