The galaxy presents as a roughly elliptical structure, elongated along its major axis. The central bulge exhibits a pronounced concentration of light, appearing a yellow-orange hue indicative of an older stellar population. The light appears to fade moving away from the bulge. There is a slight distortion of the major axis with a hint of asymmetrical distribution of luminosity, suggesting possible past or ongoing interactions. The overall smooth appearance suggests a relatively undisturbed morphology. There are some subtle blue features in the upper and lower regions of the galaxy indicating regions of possible star formation. No distinct spiral arm structure is discernible in the image.
