The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge and a gradual decrease in luminosity outwards. The color profile indicates a redder hue, suggesting a population of older stars and a lower rate of on-going star formation. There is no discernible spiral arm structure or significant dust lane obscuration visible within the galaxy. The overall morphology suggests a galaxy that has undergone significant evolution, likely with a high degree of morphological symmetry. There appears to be no major merger events. The galaxy's estimated size is relatively small.
