The galaxy presents as a fairly smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing mostly round. The core is bright, exhibiting a yellowish hue, possibly indicative of an older stellar population. Fainter, bluer light surrounds the central region, suggesting the presence of some younger stars and potentially ongoing star formation within the galaxy. There is no visual evidence of prominent spiral arms, bars, or other significant morphological features often associated with more active or dynamically disturbed systems. Overall, the galaxy appears to be relatively undisturbed and exhibits a relatively smooth light distribution.
