The galaxy presents a generally smooth, elliptical morphology. The primary body of the galaxy exhibits a high degree of circularity. A concentration of light in the central region suggests the presence of a galactic nucleus. The color profile of the galaxy indicates a higher concentration of redder wavelengths in a region that could be part of the galaxy, but may be a foreground object. The object does not appear to be undergoing a major merger, but the possibility of a minor disturbance or interaction cannot be ruled out due to the presence of asymmetry in the color distribution. There is no clear indication of spiral arm structure or significant dust lanes within the observed image. The estimated size appears relatively compact, which suggests it is a relatively small galaxy. Overall, the galaxy appears to be a relatively early-type system, exhibiting a smooth light distribution and redder overall color.
