The galaxy presents a generally smooth, elliptical morphology. Its light is dominated by yellowish hues, suggesting an older stellar population with relatively little ongoing star formation. The concentration of light is highest towards the center, gradually decreasing outwards, exhibiting no distinct spiral arm structures or prominent dust lanes. The object is largely undisturbed, with minimal signs of tidal interactions or recent mergers, though some subtle asymmetries might be present in the outer regions.
