The galaxy presents as a centrally concentrated object with an overall elliptical morphology, albeit with a slight deviation from perfect circularity. The light distribution appears relatively smooth, suggesting an older stellar population with minimal ongoing star formation. The core exhibits a subtle reddish hue, potentially indicative of dust extinction or a population of older, redder stars concentrated towards the center. Fainter, more diffuse light extends outwards from the core, forming a halo. There is a suggestion of a very slight asymmetry in the halo, perhaps indicating minor gravitational interaction or past accretion events, though no prominent tidal features or merging companions are apparent. The galaxy appears to be relatively isolated in its environment, with no immediately obvious nearby galaxies significantly perturbing its structure.
