The galaxy presents as a somewhat elliptical, though not perfectly circular, luminous entity. It appears primarily smooth in texture, lacking any discernible spiral arm structures or prominent dust lanes. There is a suggestion of a color gradient, shifting from a slightly bluer hue in the outer regions to a yellower, more concentrated glow towards the central bulge. This could indicate older stellar populations dominating the core. The apparent size is relatively compact, suggesting a small or moderately-sized galaxy. There are no immediately obvious signs of recent major mergers or tidal interactions, though subtle disturbances cannot be ruled out. It may be an elliptical galaxy. The faintness of the outer regions suggests relatively low ongoing star formation.
