The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated light distribution. The primary body is spheroidal in appearance. There is a possible second body present, but it is unclear if it is the result of a merging event or a separate, neighboring galaxy. The primary galaxy appears to be mature, as evidenced by its reddish-yellow hue, indicative of an older stellar population. Star formation appears to be relatively suppressed. There are no visible spiral arm structures or significant dust lanes, suggesting a lack of ongoing, large-scale star formation within the galaxy. Tidal disturbances in the system are only minor.
