The galaxy exhibits a generally smooth morphology. A concentrated central bulge is evident, appearing bright and somewhat circular. Fainter, diffuse extensions emanate from the core, creating a shape that is somewhere between circular and elliptical, and it seems to be closer to round than cigar-shaped. Evidence suggests some level of disturbance in the galactic structure, however, it is difficult to say if it would be characterized as minor or major. There is a secondary concentration of light offset from the primary core that may indicate the remnants of a merger or some tidal interaction. The color gradient transitions from a bluer hue at the center to a redder, more subdued tone in the outer regions.
