The galaxy exhibits a pronounced, elongated morphology, presenting a flattened elliptical shape from our vantage point. The light distribution reveals a bright, relatively concentrated central bulge, surrounded by a more diffuse, extended halo or disk. The primary axis of the galaxy is clearly defined, with a smooth gradient in luminosity moving from the core outwards. Color gradients are subtle but present, suggesting a slightly bluer tint in the outer regions compared to the redder core. There is a noticeable lack of distinct spiral arm structures or prominent dust lanes, supporting classification as an elliptical or lenticular galaxy. The overall appearance is smooth and featureless, with no obvious signs of recent major merger activity.
