The galaxy appears to be a relatively smooth, elliptical galaxy with a prominent, bright central bulge. There is a distinct, though subtle, color gradient, transitioning from a yellowish-white core to a bluer outer region. This suggests the presence of older stellar populations concentrated in the core, with relatively younger populations distributed in the surrounding regions. The galaxy exhibits a slight degree of flattening but is generally round in appearance. There is no strong evidence of a spiral arm structure or a prominent disk. While there is some patchiness in the outer regions, overall, there is a notable lack of significant morphological disturbance. It is likely a relatively massive galaxy with a low star formation rate.
