The galaxy appears to be a relatively smooth, elliptical galaxy with a diffuse and slightly oblong morphology. It exhibits a concentrated central region that gradually fades into the surrounding space, displaying a relatively featureless structure. There is no readily apparent disk-like structure. The color profile suggests a population of older stars, with light primarily emitted in the redder wavelengths. No signs of recent or ongoing major mergers are visible. Faint hints of blueish color toward the central region suggest the possibility of some star formation, although this activity appears to be low level.