The galaxy presents as a centrally concentrated object with a smooth, diffuse halo. The core exhibits a yellowish-white hue, indicative of an older stellar population. The outer regions of the galaxy display hints of blue, suggesting the presence of younger stars and ongoing, or recent, star formation activity. The galaxy appears to be largely spheroidal or elliptical in shape, with no distinct spiral arm structure readily apparent. There is a slight asymmetry or distortion in the outer regions, possibly hinting at a minor gravitational interaction or past merger event. Overall, the galaxy's morphology suggests a system dominated by older stars with pockets of recent star formation, and potentially some level of disturbance.
