The galaxy presents an elliptical morphology, appearing as a smooth, centrally concentrated distribution of light. There is a slight elongation visible, suggesting a classification towards an E4-E6 type on the Hubble sequence. The central region exhibits a bright, relatively uniform intensity, suggestive of an older stellar population. The outer regions gradually decrease in luminosity, with no apparent spiral arms or distinct features. Color gradients are subtle, with a hint of bluer tones in the outer halo potentially indicating some ongoing star formation. The overall structure appears undisturbed, with no obvious signs of recent mergers or tidal interactions.
