The galaxy presents a generally smooth appearance with a central concentration of light. The shape is elliptical with a degree of roundness; there's little indication of spiral arms or a well-defined disk structure. Faint blue hues on the periphery might indicate regions of younger star formation. There appears to be evidence of minor disturbances or asymmetries in the galaxy's morphology, indicating possible interactions or mergers in its past. The overall color profile is consistent with an older stellar population.
