The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution appears centrally peaked, with a gradual falloff in intensity outwards. There is a noticeable yellow-orange hue to the galaxy, particularly within the central region. This suggests an older stellar population with a lower rate of star formation. There is very little evidence of spiral arm structures, or significant dust lanes. The overall shape is generally round. There are no obvious signs of ongoing major mergers or tidal disturbances.
