The galaxy appears as a moderately luminous object, exhibiting an overall elliptical morphology. Its color profile indicates a relatively evolved stellar population. The galaxy presents a generally smooth appearance, with a central concentration of light suggesting a bulge component. Subtle deviations from perfect ellipticity are visible, potentially indicative of minor tidal interactions or internal structures. The object's spatial extent is relatively compact, corresponding to a moderate physical size given its distance implied by the redshift. There is no obvious spiral arm structure, implying a classification towards early-type galaxies. It also shows some evidence of a minor merger or disturbance, potentially influencing its overall shape and structure.
