The galaxy presents as a relatively compact object. Its dominant color is a yellowish-orange hue, suggesting a stellar population comprised predominantly of older stars. A subtle green tinge surrounding the core may indicate the presence of some ongoing, albeit limited, star formation activity. The galaxy's overall morphology appears smooth and featureless, showing little to no evidence of spiral arms or other distinct structures. Its ellipticity appears modest, somewhere between round and cigar shaped. There is no strong visual evidence of any ongoing major merger events, but the possibility of a minor disturbance cannot be entirely ruled out.
