The galaxy presents a largely smooth morphology, exhibiting minimal discernible features suggestive of spiral arms or a distinct disk structure. It appears nearly round in shape, showing only a slight deviation from perfect circularity. The color profile suggests a higher concentration of older stellar populations, contributing to a reddish-yellow hue, with a possible indication of reduced ongoing star formation. There's no immediate visual evidence of major mergers or significant tidal disturbances affecting the galaxy's overall structure. The galaxy has an estimated size of approximately 7 kpc across, based on observed measurements.
