The galaxy appears to be a relatively smooth elliptical galaxy, characterized by a centrally concentrated bulge. The light distribution gradually decreases from the core outwards, exhibiting a fairly regular profile. The galaxy appears somewhat flattened. There is some minor indication of possible disturbance, or potentially some internal dust lanes but nothing too major. Overall, the morphology suggests a more evolved system, with the majority of star formation having ceased. The colors show a general lack of blue light, indicating an older stellar population.
