The galaxy presents as a somewhat elongated, elliptical morphology. The central region exhibits a concentrated, bright core. The light profile appears smooth with a gradual decline in intensity from the core outward, suggesting a relatively even distribution of stellar populations. A faint disc is present in the outer regions. There is no visual evidence of spiral arm structure or significant dust lanes. The galaxy appears mostly undisturbed with no obvious signs of a major merger event, although some minor disturbances could be present. The color is relatively homogenous across the galaxy, trending towards redder wavelengths in the central bulge and slightly bluer in the faint disc. Overall, the galaxy appears to be a massive, relatively evolved system.
