The galaxy presents as a generally smooth, elliptical object, displaying a concentrated central bulge. Its shape is somewhat elongated, approximating a cigar shape. There is a noticeable lack of distinct spiral arm structures or prominent features typically associated with disk galaxies. The light distribution appears relatively uniform across the galaxy, with a gradual decrease in intensity towards the outer regions, suggesting a well-mixed stellar population. There are no immediately apparent signs of major merger activity or significant tidal disturbances impacting the galaxy's overall structure. The color profile indicates a dominance of older stellar populations, which accounts for the redshift. This is consistent with characteristics of a relatively massive galaxy with moderate star formation occurring.