The galaxy presents as a somewhat elliptical structure, approximately 10.7 kpc in radius. The central region exhibits a higher concentration of luminosity, appearing bright yellow in color. The yellow color is likely representative of an older stellar population. Progressing outwards from the core, the galaxy's luminosity decreases gradually. There appears to be a faint disk with some features. The overall morphology suggests a galaxy with minimal ongoing star formation. There are no obvious signs of a major merger or significant tidal disturbances in this image. 
