The object appears to be a galaxy at a considerable distance, with an estimated redshift of approximately 0.285. Morphologically, it presents as a relatively smooth, centrally concentrated object with a generally elliptical shape. There are no obvious spiral arm structures or significant dust lanes visible. The galaxy's light profile indicates a gradual decline in surface brightness from the core outwards. Color gradients suggest a slightly bluer outer region transitioning towards a redder core. The object does not display any strong signs of tidal disturbances or ongoing major mergers.
