The galaxy presents as a spheroid shape. It exhibits a bright, concentrated central bulge, appearing yellowish in color. The outer regions of the galaxy appear fainter and display a slightly elongated or cigar-shaped morphology. Some indication of possible faint spiral arms can be observed. There are no obvious signs of ongoing major merging events or tidal tails, although some minor disturbances or asymmetries within the disk could be present. Overall, this appears to be a relatively undisturbed galaxy, potentially an elliptical or a late-type spiral galaxy with a dominant bulge. The galaxy is estimated to be very massive, with a high rate of star formation.
