The galaxy presents a predominantly elliptical morphology, appearing largely smooth and centrally concentrated. It exhibits a yellowish-orange hue, suggesting a stellar population dominated by older, redder stars. There may be a lack of significant recent star formation, as evidenced by the absence of prominent blue regions typically associated with younger, hotter stars. While a distinct disk structure is not immediately apparent, there appears to be some form of feature. Minor disturbances possibly indicative of a past interaction are observable, though these are not overtly pronounced. The galaxy appears relatively round in overall shape.
