The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The color profile suggests an older stellar population, primarily redder in the core region, indicative of evolved stars. Some faint blue patches are present in the outer regions, potentially hinting at localized, low-level star formation activity or a contribution from a younger stellar population. The galaxy appears relatively undisturbed, with no obvious signs of a major merger or significant tidal interactions. The elongation appears to be in between round and cigar shaped. Based on color distribution and smooth appearance, the galaxy is likely a relatively massive system. 
