The galaxy presents as a somewhat elliptical, disk-like structure with a relatively smooth appearance. There is evidence of a central bulge, which appears slightly yellowish, possibly indicating an older stellar population concentrated in the core. Extending outwards from the central region, a fainter, bluish halo or disk is visible. The blue color suggests ongoing star formation within this outer region. There is a slight asymmetry or possible minor disturbance in the galaxy's overall structure. Although appearing relatively undisturbed at first glance, careful observation reveals a hint of irregularity, possibly indicating a past interaction or minor merger event.
