The galaxy presents as a luminous, elliptical-shaped object. The central region displays a concentrated and bright core, suggesting a high stellar density, potentially indicative of an older stellar population. This core appears to transition smoothly outward, with the light gradually diminishing towards the galaxy's periphery. Subtle color variations are discernible within the galaxy; the core exhibits a slightly yellow hue while the outer regions show a hint of bluer tints. This may suggest ongoing, albeit moderate, star formation in the outer regions. The overall morphology leans toward a smooth and largely undisturbed structure, although there is some hint of a mild disturbance in the outer regions. The galaxy's orientation is such that we observe it at a slight angle, offering a somewhat oblique view of its shape.
