The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its core exhibits a bright, yellowish-white luminosity, suggesting a high density of older stellar populations. Fainter, diffuse extensions radiate outwards from the core, presenting a slight bluish tinge on one side, potentially indicating regions of more recent, albeit subdued, star formation activity. The overall structure lacks any distinct spiral arms or bar features. There is no evidence of ongoing major merger activity, though subtle asymmetries in the outer regions may hint at minor interactions or tidal disturbances in its past. The galaxy appears relatively isolated in its immediate vicinity.
