The galaxy presents as a well-defined elliptical system, appearing largely smooth in texture. The light distribution suggests a central bulge that dominates the overall luminosity. This bulge exhibits a yellowish hue, suggestive of an older stellar population. Moving outwards from the bulge, there is a subtle decrease in surface brightness, and the color appears slightly bluer, though still relatively uniform. There is no apparent dust lane or spiral arm structure visible, and the overall morphology is consistent with an early-type galaxy at a considerable distance. The galaxy exhibits a moderate ellipticity, being elongated along one axis. There is no apparent sign of ongoing major mergers or significant tidal disturbances.
