The galaxy presents a generally smooth and elliptical morphology. A distinct central bulge dominates the galaxy's structure, exhibiting a concentrated, bright, yellowish hue that suggests an older stellar population within. The luminosity gradually decreases outwards from the core into a more diffuse halo. There is very little evidence of spiral arms or significant dust lanes. A slight blue tint is visible in the outer regions, potentially indicative of some ongoing, albeit low level, star formation. There appear to be some minor disturbances, potentially indicative of a past merger event. Overall, the galaxy appears to be a relatively evolved system.
