The galaxy presents as a relatively smooth, centrally concentrated object. It appears elliptical in shape, exhibiting a high degree of rotational symmetry. The galaxy does not display prominent spiral arms or a well-defined disk structure. There is a subtle color gradient, with the central regions appearing slightly redder than the outer regions. No significant tidal features or signs of recent major merger activity are discernible. The galaxy appears to be relatively isolated, with no obvious companion galaxies in close proximity. Overall, the galaxy's morphology suggests a spheroid-dominated system, likely an elliptical or lenticular galaxy, with a high degree of internal order.
