The galaxy presents a somewhat smooth appearance with a central bulge that is more luminous and appears to be composed of older stellar populations, indicated by its yellowish hue. The morphology is best described as an elliptical shape with a clear elongation along one axis; this aligns with a moderate probability that the galaxy is more "cigar shaped" than spherical. There is some evidence of a disk-like structure, but the central bulge dominates the overall appearance. There are no obvious signs of ongoing major mergers or significant tidal disturbances in the immediate vicinity, although subtle asymmetries in the outer regions could suggest minor gravitational interactions in the past. Faint blue tinges in the outer regions possibly suggest ongoing star formation. The size is relatively compact.
