The galaxy presents a somewhat elliptical morphology, appearing largely smooth and lacking prominent spiral arms. The luminosity distribution appears centrally concentrated, with a gradual falloff in surface brightness towards the outer edges. The color profile indicates a population of older stars, with a dominant redder hue. There is a slight indication of tidal disturbances or asymmetries in the outer halo, suggesting a potential past or ongoing interaction with another galaxy, although no major merger is apparent. Overall, this galaxy appears to be a relatively evolved system with little to no active star formation.
