The galaxy presents an elongated morphology, appearing cigar-shaped in its overall form. A smooth, centrally concentrated bulge is evident, dominating the light profile, with a color gradient indicating older stellar populations in this region. Emanating from the central bulge is a faint, elongated disk. This disk exhibits a bluer hue compared to the bulge, implying the presence of younger, star-forming regions. There appears to be a subtle perturbation or minor disturbance in the disk, although no significant merger features are readily apparent. Overall, the galaxy's morphology suggests a transition object, with characteristics intermediate between a pure elliptical and a spiral galaxy.
