The galaxy presents a predominantly smooth morphology, with a centrally concentrated bulge. The overall shape appears somewhat elliptical, exhibiting a deviation from a perfectly circular form but lacking any pronounced elongation. There is evidence of a disk component contributing to the galactic structure. The light distribution indicates a relatively homogenous stellar population across the visible region of the galaxy, with a subtle color gradient from a yellow core to a whiter halo. There is no compelling evidence of ongoing major mergers or significant tidal disturbances.
