This galaxy appears as a relatively smooth, rounded object with an elliptical morphology. There is little evidence of spiral arms or significant disk features in this image. The galaxy presents with a concentrated central bulge, gradually fading towards its outer edges. Color gradients suggest a higher concentration of older stellar populations in the galactic core, becoming bluer in the outskirts, which may indicate ongoing or recent star formation, though relatively low in intensity. There is no strong evidence of major mergers or tidal disturbances in this image, though some minor irregularities may be present. Overall, the galaxy exhibits characteristics typical of an early-type galaxy undergoing passive evolution, potentially at a redshift of approximately 0.26. Its estimated size is approximately 6 kpc in radius, and its luminosity is high.
