This galaxy appears to be a relatively compact object, exhibiting a centrally concentrated light profile. A bright core or nucleus is visible, indicating a higher density of stars in this region. Surrounding this core is a diffuse, extended halo or bulge. The shape of the galaxy appears somewhat irregular and not completely smooth, potentially indicating gravitational interactions, minor disturbances, or ongoing mergers. There may be some faint tidal features or debris visible in the surrounding area, suggesting possible ongoing interactions. There is a lack of defined spiral arms or significant disk-like features.
