The galaxy presents as a relatively compact object, displaying a generally elliptical morphology. It appears moderately bright, with a core region that exhibits higher luminosity. The light distribution suggests a centrally concentrated structure with a gradual decrease in intensity outwards.

A subtle color gradient is observed, with the central region appearing slightly more yellowish, possibly indicating an older stellar population. Faint bluish hues are noticeable in the outer regions, potentially indicating the presence of younger, hotter stars and ongoing, but potentially low-level, star formation. There are hints of slight asymmetry or minor disturbances in the outer regions, but the galaxy does not appear to be undergoing a major merger or violent interaction. The galaxy presents a smoothness in its overall structure, which is not uncommon for galaxies of its type.
