The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light distribution suggests a lack of significant spiral arm structure or prominent dust lanes. The core exhibits a yellowish hue, possibly indicative of an older stellar population dominating the central region. The outer regions appear more diffuse, with a slight color gradient towards redder tones. There is no obvious evidence of ongoing major mergers or strong tidal disturbances. The galaxy's apparent size is relatively small, consistent with it being at a considerable distance. There is a suggestion of minor interactions with smaller objects nearby. The galaxy is likely relatively massive, with a moderate rate of star formation. The specific star formation rate suggests it is primarily a quiescent galaxy.
