The galaxy appears to be a yellowish elliptical, with a smooth, centralized light distribution. The core exhibits a high surface brightness, gradually decreasing towards the outer regions. There is a slight elongation or flattening, suggesting it may not be perfectly spherical. There is a faint hint of disturbance, possibly due to a past or ongoing interaction, but its overall structure remains largely undisturbed. There is limited color variation, with the galaxy displaying a consistent yellow hue, indicative of an older stellar population and low star formation rate. 
