The galaxy presents as a relatively smooth, elliptical morphology. There's a bright, concentrated central bulge exhibiting a yellowish-orange hue, potentially indicating an older stellar population. The radial light profile appears to decrease smoothly outwards from the core, showing no distinct spiral arm structures or prominent dust lanes. The overall shape seems roughly round, though slightly elongated. There are possible indications of minor disturbances or tidal features in the outskirts, suggesting past or ongoing interactions with other galaxies. The galaxy appears to be relatively massive. Star formation may be present, though subdued.
