The galaxy presents as a somewhat elliptical, disc-like structure, appearing approximately 10 kpc in radius. A central bulge exhibits a concentrated, bright, yellowish-orange hue, suggesting a high density of older stellar populations. Surrounding the bulge is a fainter, bluer disc. The disc exhibits some irregularities, potentially indicating minor gravitational disturbances or interactions. There appears to be ongoing star formation, indicated by the bluer colour, but the rate of star formation is not high. The galaxy shows no strong evidence of a recent major merger or tidal features. The overall morphology is consistent with a transitionary phase between a spiral and elliptical galaxy. There is likely a supermassive black hole, of approximately 10^11 solar masses, present at the center of the central bulge.
