The galaxy presents as a relatively smooth, elliptical structure. The central bulge exhibits a yellowish hue, suggesting an older stellar population and potentially lower levels of ongoing star formation. The isophotes are generally well-behaved, with a slight elongation that could indicate a transition between a spherical and a more flattened elliptical morphology. There are some hints of a faint, diffuse halo extending beyond the central bulge, but the limited resolution makes it difficult to ascertain its detailed structure or extent. Visual inspection suggests the object is likely a relatively massive galaxy with a redshift of 0.189410. Overall, it appears to be an early-type galaxy with a notable spheroidal component, potentially residing in a more quiescent state.