The galaxy presents as a slightly elongated, smooth object with a diffuse halo. It exhibits a color gradient, transitioning from a concentrated, yellowish core to a bluer, less defined outer region. There is a noticeable absence of distinct spiral arm structures or prominent dust lanes. The galaxy appears relatively undisturbed, showing no strong signs of tidal interactions or ongoing mergers. The overall light profile suggests a dominant bulge component and a moderate disk presence. The color implies ongoing, but relatively low, star formation.
