The galaxy presents an overall smooth morphology, with a centrally concentrated, bright, and slightly elongated core. There is minimal evidence of distinct spiral arm structures or significant star-forming regions within the visible portion of the galaxy. The color profile appears to be relatively uniform across the galaxy, exhibiting a subtle gradient towards redder hues in the central region and a gradual shift towards bluer colors within the outer regions. This suggests that the galaxy is populated primarily with an older stellar population in the central region and a possible younger population in the outer regions. The shape is generally elliptical, with a minor deviation from perfect circularity. There are no obvious signs of major mergers or tidal disturbances in the immediate vicinity, although a very slight asymmetry in the outer halo cannot be fully ruled out. Overall, the galaxy appears to be an evolved system, possibly an elliptical or lenticular galaxy viewed at a significant distance.
