The galaxy presents a generally smooth, elliptical morphology with no apparent spiral arm structure. The central bulge region is dominant and exhibits a concentrated, bright, yellowish hue, suggesting a population of older stars. The galaxy's light profile appears relatively even, lacking significant knots or clumps of star formation. There is a subtle color gradient from the core outwards, shifting towards slightly redder tones, further indicating an aging stellar population and a possible decline in recent star formation. The overall structure seems undisturbed, without any obvious signs of tidal interactions or major mergers. The object's apparent shape is somewhat elongated, although not significantly cigar-shaped. 
