The galaxy exhibits an elliptical morphology, appearing largely smooth and featureless. There is a concentrated central bulge exhibiting a bright yellowish-white hue, possibly indicating a population of older stars. The galaxy gradually fades outward from the core into a fainter halo. No spiral arm structures are visible, nor is there any obvious evidence of ongoing merging activity or strong tidal disturbances. The ellipticity is low, indicating it is closer to being circular than cigar-shaped. Overall, the galaxy seems to be an early-type galaxy.