The galaxy appears as an elliptical or lenticular type, exhibiting a smooth, diffuse morphology with a centrally concentrated bulge. No distinct spiral arm structures are visible. There is an indication of a close companion object, possibly another galaxy in the process of merging or interacting with the primary galaxy. The primary galaxy displays a somewhat rounded shape, though not perfectly spherical, with a slight elongation. There are no strong indicators of active star formation regions, such as bright blue knots or HII regions, suggesting a relatively quiescent or passive state. The color profile indicates a redder overall color, consistent with an older stellar population dominated by evolved stars, although its absolute magnitude places it as a large galaxy. There is a faint, extended halo of stars surrounding the main body. There is a slight but noticeable visual irregularity, indicating some form of disturbance to the system, possibly from the close companion, though the galaxy would still be considered relatively undisturbed overall. 
