The galaxy presents as a well-defined, elongated structure. The morphology is generally smooth, exhibiting a prolate spheroid shape. It is oriented with its major axis extended across the frame. The central region displays a concentrated luminosity profile, suggesting a significant stellar population density. The outer regions gradually fade, transitioning to a fainter halo. There's a hint of color variation, with the core appearing more yellow or red-shifted, possibly indicating an older stellar population, and the outer regions exhibiting bluer hues, suggesting the presence of younger stars. No apparent spiral arms or major disturbances are visible. The overall appearance suggests an elliptical galaxy, possibly of type E5-E7, seen at an angle.
