The galaxy appears as a centrally concentrated object, likely a spiral, with a relatively smooth overall structure. It exhibits an elongated morphology, approaching a cigar-like shape, with a bright central bulge. Faint, diffuse arms or features can be tentatively identified extending from the central region. There are slight color variations across the galaxy, with the central bulge appearing more yellowish, potentially indicating an older stellar population, and the outer regions appearing bluer, suggesting younger stars. There is no clear indication of any major ongoing merger activity or strong tidal disturbances, though minor disturbances cannot be ruled out. The galaxy's overall appearance suggests that it may be undergoing a period of relatively quiescent evolution, with ongoing star formation at a modest rate.
