The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The core exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outward from the core, the galaxy shows a gradual decrease in surface brightness. The overall shape deviates slightly from perfectly circular, appearing somewhat elongated or cigar-shaped. There is no obvious spiral structure, strong dust lanes, or tidal tails apparent in the image. The galaxy appears to be relatively isolated, with no obvious signs of major interaction or merging events. Subtle disturbances might be present within the faint outer regions.
