The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There is no clear evidence of spiral arms or a prominent disk structure. The light profile decreases gradually from the center, suggesting a well-mixed stellar population. Color gradients are subtle, but the central region exhibits a slightly yellower hue, potentially indicating older stars or a higher concentration of dust in the core. No major disturbances or tidal features are readily apparent, suggesting that it is not currently undergoing a major merger event, though subtle asymmetries may be present. The galaxy appears relatively isolated.
