The galaxy presents a centrally concentrated morphology. The core region is characterized by intense luminosity, displaying a distinct blue hue, suggestive of a significant population of young, hot stars or an active galactic nucleus. A faint, diffuse halo surrounds the core. The overall structure appears somewhat irregular, with subtle extensions or tidal features visible. These features indicate the possibility of past or ongoing gravitational interactions with another galaxy. The light profile appears relatively smooth, but there are slight irregularities present that may indicate the presence of a disk or spiral arms.
