The galaxy presents as a single, relatively smooth object. It exhibits a concentrated central region, suggestive of a bulge. The overall color appears somewhat blueish, particularly in the outer regions, which could indicate the presence of younger stellar populations and ongoing star formation. There is no apparent disk structure or spiral arms visible, leading to a classification of the galaxy as elliptical, or perhaps an early-type spiral lacking well-defined arms. Its morphology is generally undisturbed, without any significant signs of tidal interactions or recent mergers, appearing as an isolated system. The shape is slightly elongated, neither perfectly circular nor exceptionally flattened.
