The galaxy presents as an elliptical morphology with a smooth, relatively featureless structure. The light distribution suggests a high degree of central concentration, characterized by a bright, yellowish core. The light gradually diffuses outwards from the core, with a radial decrease in intensity. There is very little evidence of spiral arm structure or significant dust lanes. The overall shape is almost perfectly round, with only a slight deviation from a circular profile. The color gradient suggests an older stellar population dominating the central bulge, which is consistent with low levels of on-going star formation. There is very little evidence of any recent or ongoing mergers or tidal disturbances.
