The galaxy appears as a generally smooth, elliptical structure. Its morphology is primarily dominated by a central bulge that exhibits a bright, concentrated luminosity, suggesting a high stellar density. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness. While the overall form appears smooth, subtle color variations are present. The inner regions exhibit a yellowish hue, possibly indicative of an older stellar population. There is a slight elongation, giving it a somewhat cigar-shaped appearance, rather than being perfectly spherical. There is little to no evidence of distinct spiral arms or prominent dust lanes, furthering the classification towards the elliptical end of the Hubble sequence. No signs of ongoing major merger activity are apparent; any disturbances are at most minor.
