The galaxy appears to be a relatively smooth, centrally concentrated object. Its morphology is largely elliptical, with an estimated diameter of approximately 4 kpc. The galaxy exhibits a primarily blue hue, suggesting the presence of younger stellar populations and ongoing, yet suppressed, star formation activity. There is no strong visual evidence of spiral arm structures or significant dust lanes. The object is relatively undisturbed, showing no major signs of tidal interactions or recent merger events. Faint, extended emission may be present, forming a somewhat diffuse halo surrounding the galaxy's core.
