The galaxy presents as an elongated, ellipsoidal structure. The central region exhibits a yellowish hue, suggesting an older stellar population or dust obscuration. Proceeding outward from the core, the color transitions to a bluer shade indicating younger star formation. The galaxy appears relatively smooth in texture, with no readily discernible spiral arm structures or prominent dust lanes. The light distribution along the major axis appears to gradually diminish with increasing distance from the center, indicating a diffuse outer halo or envelope. No clear signs of tidal tails or recent merger activity are immediately apparent in the image, although slight disturbances may be present. The overall morphology indicates that the galaxy may be an elliptical or lenticular type, with a considerable amount of mass present. There is moderate ongoing star formation based on the bluer color of its outer parts.
