The galaxy presents a somewhat elliptical morphology. It appears relatively smooth in texture, with no prominent spiral arm structures or significant dust lanes visible. The core region exhibits a brighter, concentrated luminosity suggesting a possible central bulge. The galaxy displays a color gradient, transitioning from a bluer hue in the central regions to a more reddish tone towards the outer edges. This may indicate differing stellar populations, with younger, hotter stars concentrated centrally, and older, cooler stars dominating the periphery. There are subtle signs of possible tidal disturbances or minor asymmetries. The object appears to be a relatively low-mass galaxy with a modest rate of star formation.
