The galaxy appears to be a relatively small, distant object, characterized by an elongated, cigar-shaped morphology. Its light is primarily concentrated in a smooth, central bulge, exhibiting a yellow-orange hue. Extending outwards from the central bulge, there's a fainter, disk-like structure visible, showing subtle blue tones, possibly indicative of younger stellar populations. There is no strong evidence of a major ongoing merger or tidal disturbances, though a slight asymmetry in the outer regions cannot be entirely ruled out. Overall, the galaxy presents characteristics consistent with a transitioning morphology, potentially evolving from a late-type spiral towards an earlier-type lenticular or elliptical galaxy.
