The galaxy appears as a centrally concentrated, elliptical-like object. It exhibits a smooth morphology with minimal discernible features, such as spiral arms or a bar structure. The galaxy appears nearly circular in shape. There's no apparent evidence of ongoing or recent major mergers or tidal disturbances in the immediate vicinity. The color profile suggests a population of older stars, resulting in a reddish hue. Star formation appears relatively low, contributing to the lack of blue colors typically associated with younger, hotter stars.
