The galaxy appears to be an elliptical type, exhibiting a smooth, centrally concentrated light distribution. It is largely featureless, lacking prominent spiral arms or a distinct disk structure. The shape is generally round, though there is a slight elongation. The core of the galaxy shows a strong concentration of light, and the color suggests a population of older stars with relatively little ongoing star formation. There is no obvious evidence of any major disturbances or ongoing mergers. A slight asymmetry in the outer regions might suggest a past minor interaction, but this is not clearly defined.
