The galaxy appears as a single, concentrated body of light, suggesting an elliptical morphology. The light distribution is centrally concentrated with a smooth, radial falloff in brightness. There is a dominant central bulge that appears largely featureless, and there are no visible spiral arms or a distinct disk-like structure. The galaxy exhibits a color gradient, being more yellow-white towards the center and shifting slightly redder in the outer regions. This color profile is consistent with an older stellar population and a cessation of significant star formation activity. There are no obvious signs of tidal interactions or ongoing mergers affecting the galaxy's morphology.
