The galaxy presents an overall elliptical morphology, appearing elongated with a cigar-like shape. It exhibits a smooth, concentrated central bulge that dominates the light profile. There is evidence of a faint, diffuse disk surrounding the bulge. The galaxy's color index suggests a population of older stars, with the dominant light originating from the redder end of the spectrum. No major disturbances or signs of ongoing mergers are readily apparent, though a minor disturbance cannot be ruled out. Based on its apparent shape and color profile, the galaxy is likely an early-type spiral or elliptical.
