The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. It exhibits a bright, relatively compact core, surrounded by a more diffuse halo. There's a subtle color gradient, shifting from a bluer hue in the central regions to a redder tint towards the outer edges. This could indicate varying stellar populations, with younger, hotter stars concentrated in the core and older, cooler stars dominating the outskirts. There is little evidence of distinct spiral arms or prominent dust lanes; the overall structure suggests a relatively evolved system. The object has intermediate roundness, it doesn't look totally spherical, nor does it look cigar shaped. There is no current apparent signs of any merging with other objects. 
