The galaxy presents as a relatively symmetrical, moderately concentrated system. The central region appears bright and somewhat unresolved, displaying a yellowish-white hue, suggesting a population of older stars. A faint, diffuse halo surrounds the core, extending outwards. This outer region exhibits a subtle bluer tint, perhaps indicating the presence of younger stars or ongoing star formation. The galaxy appears to be relatively smooth in texture with hints of arm structures, though they are ill-defined and lack the high contrast often seen in grand design spirals. No significant dust lanes or prominent star-forming regions are readily apparent in the image, and no clear signs of tidal disturbances or ongoing major merger events are visible.
