The galaxy presents an elliptical morphology, appearing largely spheroidal in shape. Its core exhibits high luminosity, indicative of a dense stellar population. The light distribution transitions smoothly outward from the nucleus, with the outer regions displaying a lower surface brightness. There is evidence of weak structure and minor disturbances suggesting potential past or ongoing interactions. Color gradients are subtle, trending towards a slightly redder hue in the outer regions compared to the yellower core. The overall structure suggests a relatively evolved system with minimal recent star formation, though some low level activity cannot be ruled out. The galaxy presents a substantial mass as calculated with a redshift of 0.218509.
