The galaxy presents as a largely featureless, elliptical morphology. The light distribution suggests a smooth, centrally concentrated profile with a gradual decline in surface brightness from the core outwards. The color gradient exhibits a yellowish hue in the central region, transitioning to a slightly bluer periphery. This could be due to varying stellar populations, with older, redder stars dominating the core and younger, bluer stars existing in the outer regions of the galaxy, or differences in metallicity. No distinct spiral arms, bar structures, or prominent dust lanes are apparent in this image. The overall form is fairly regular, with a slight elongation, suggesting a classification somewhere between E2 and E4 on the Hubble sequence. There appears to be no indication of major tidal disturbances or ongoing merger activity, although minor asymmetries cannot be ruled out at this resolution. The substantial redshifting is potentially indicative of an older, more passively evolving system with relatively low star formation activity.
