The galaxy presents a generally elliptical morphology with a high degree of central concentration. The light distribution suggests a bulge-dominated system with a smooth, diffuse halo extending outwards. There appears to be some distortion or asymmetry in the outer regions of the galaxy, hinting at a possible interaction or recent merger event. The galaxy exhibits a yellow-reddish hue, characteristic of an older stellar population with relatively little ongoing star formation. Within the central region, there are what appear to be two bright points of light.
