The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration indicated by a bright core. The shape deviates slightly from perfect roundness, appearing somewhat elongated. Subtle color gradients are observed, with the central region exhibiting a yellower hue, possibly indicative of an older stellar population. Fainter, bluer regions are detected in the outskirts of the galaxy, suggesting ongoing, albeit low-level, star formation activity. There's a hint of disturbance, possibly from a minor interaction with another galaxy or recent gas accretion. This is indicated by a very slight asymmetry in the outer isophotes. No distinct spiral arm structure or prominent dust lanes are visible in the image.
