The galaxy presents as a diffuse, elliptical-like object with a generally smooth appearance. The core appears brighter and more concentrated, with a gradual fading of luminosity towards the outer edges. The primary color is a yellowish-orange hue, suggesting an older stellar population and a relatively low rate of ongoing star formation. There are hints of faint blue regions intermixed, particularly on one side, potentially indicative of some younger, hotter stars. The overall morphology suggests the galaxy is an early-type spiral or elliptical galaxy. There is a possibility of minor tidal disruption or interaction based on some subtle asymmetries in the outer halo and the slight hint of a tail.
