The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. A bright, yellowish core is evident, transitioning outward to a more diffuse halo of bluer light. No distinct spiral arms or prominent dust lanes are discernible. The overall color suggests a mix of stellar populations, with older, redder stars likely dominating the central region and a younger, bluer population present in the outer regions. The general structure suggests a galaxy undergoing, or having recently undergone, a period of star formation. There appears to be some minor disturbance visible, possibly indicating an ongoing or recent interaction with another galaxy, or a minor merger event. The galaxy is neither perfectly round nor elongated, appearing slightly closer to a round morphology.
