The galaxy presents a largely smooth, elliptical morphology. It displays a concentrated central bulge, exhibiting a bright yellowish-white hue, suggesting a population of older stars.  Moving outward from the core, the color transitions to a slightly bluer shade. The galaxy does not show prominent spiral arm structures or a well-defined disk, rather appearing as a somewhat diffuse, spheroidal object.  A slight asymmetry is present, with a minor disturbance in the galaxy's outskirts, potentially indicating a minor interaction or past merger event. The overall smoothness and lack of prominent features are consistent with a galaxy dominated by an older stellar population with an intermediate mass.
