The galaxy appears as a single, concentrated object with a smooth light distribution. There is evidence of possible tidal distortions. The galaxy exhibits a moderate degree of ellipticity. The galaxy's light profile is concentrated towards the center, with the outer regions fading gradually into the background. There is an orange hue indicating the presence of relatively older stellar populations within the system, particularly in the central region. There is very little blue color, suggesting minimal recent star formation. The morphology is indicative of a spheroidal galaxy.