The galaxy presents a smooth, elliptical morphology, displaying a concentrated central bulge that gradually fades into a less defined outer halo. The color profile suggests a relatively older stellar population, with a discernible shift towards redder wavelengths. There is no visible evidence of prominent spiral arms or active star-forming regions; the overall structure appears quiescent. Slight asymmetry may hint at minor gravitational interactions or a previous merger event, though no substantial tidal features are apparent. The galaxy's shape deviates slightly from perfectly spherical, exhibiting an elongated, somewhat cigar-shaped form.
