The galaxy exhibits a smooth, elliptical morphology. Its central bulge is bright and concentrated, with a noticeable decrease in luminosity moving outwards. The shape appears close to round, with minimal deviation toward a cigar-like form. There are no obvious signs of strong tidal disturbances or ongoing mergers; only a few minor irregularities are detected in the outer regions. The color gradient indicates a largely older stellar population, with a redder hue in the bulge, and a bluer one in the disc. Star formation rate appears low, which is consistent with the color. The galaxy is of intermediate size, neither particularly compact nor exceptionally large.
