The galaxy presents as an elliptical type with a smooth, centrally concentrated bulge. A subtle color gradient is observed, shifting from a yellowish hue in one region to a bluish tint in another region. This could be indicative of variations in stellar population or dust content across the galaxy. While difficult to definitively assess from this image, there appears to be some degree of tidal disturbance, or possibly an ongoing minor merger event, the galaxy could be interacting with another galaxy, or possibly another galactic body. The overall shape appears elongated with a bar structure, but its true nature is obscured by the limited resolution. The color index indicates a relatively evolved stellar population.
