The galaxy presents as a diffuse, elliptical morphology. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars or possibly an active galactic nucleus. The overall color appears reddish-yellow, which could indicate an older stellar population with a relatively low rate of current star formation. There is little evidence of spiral arms or significant dust lanes, pointing towards a smoother stellar distribution. The shape deviates noticeably from perfectly round, appearing somewhat elongated or cigar-shaped. There is no visual indication of any major ongoing merger events or significant tidal disturbances. The galaxy appears relatively isolated and undisturbed in this image.
