The galaxy presents a largely smooth, elliptical morphology with a notable lack of defined spiral arm structures. The light distribution appears relatively uniform across the galaxy, with a concentrated central bulge that gradually fades towards the outer edges. The object exhibits a mild elongation, with a shape somewhere between round and cigar-shaped. There is no obvious evidence of any ongoing major merger activity or significant tidal disturbances impacting the system's overall structure. A subtle color gradient exists, hinting at variations in stellar populations, with the central region appearing slightly redder compared to the bluer hues of the outer regions. This is indicative of older stars concentrated in the center. The blue tint on the outskirts suggests some degree of recent star formation, although the rates appear to be overall quiescent. In essence, this galaxy appears to be a mature system, gravitationally stable, and undergoing only limited star formation.
