The object appears to be an elliptical galaxy at a considerable distance, with an estimated redshift of approximately 0.23. Morphologically, it appears relatively smooth and round, with no discernable spiral arm structure or bar. The galaxy exhibits a centrally concentrated light profile, characteristic of elliptical systems, with the intensity decreasing gradually towards the outer edges. The color profile suggests a population of older stars, as indicated by the greater brightness in redder wavelengths, with a slight bluer hue closer to the central region indicating ongoing star formation. There is no apparent evidence of major mergers or significant tidal disturbances in the image, though some minor asymmetries in the outer isophotes might suggest some recent or ongoing interaction.
