The galaxy appears as an elongated, smooth structure. There is a slight color gradient from the center outwards, with the central region having a yellower hue and the outer edges appearing slightly bluer. No distinct spiral arms or dust lanes are discernible. The galaxy's overall shape suggests a classification leaning towards an elliptical morphology but has some slight characteristics of a lenticular galaxy. There are no significant signs of ongoing major mergers or tidal disturbances. Faint and subtle irregularities might suggest minor gravitational interactions. The overall light distribution is relatively smooth and concentrated toward the center, indicating a relatively evolved stellar population, and is experiencing minimal star formation.
