This galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with no immediately discernible spiral arms or strong bar structure. The core is relatively bright and concentrated, displaying a yellowish hue, which could indicate an older stellar population with a diminished rate of ongoing star formation. Moving outward from the center, the galaxy becomes more diffuse, gradually fading into the background sky. There might be a slight flattening, suggesting a possible disk component viewed at a shallow angle. Minor asymmetries are present, however, do not indicate a major ongoing merger, only a small disturbance. Overall, the galaxy appears relatively undisturbed, potentially an isolated galaxy evolving passively.
