The galaxy presents as a centrally concentrated system, with a smooth, diffuse light distribution. It exhibits an elliptical morphology, with the 'roundness' being somewhere in between perfectly round and an elongated cigar shape. The core appears to be dominated by older stellar populations, judging by the yellowish-orange hue. There are no prominent spiral arms or features indicative of active, ongoing star formation visible in this image. Faint, diffuse outer regions suggest a possible extended stellar halo. There is no strong evidence of a major merger event. Any disturbances appear to be minor if present at all. The overall structure suggests a mature galaxy, likely nearing the end of its evolutionary cycle.
