The galaxy presents a generally smooth morphology, with a dominant, concentrated central bulge. The light distribution suggests a relatively high degree of spherical symmetry, leaning towards an elliptical classification. Faint, diffuse extensions are visible surrounding the main body, which may indicate a tenuous stellar halo, but this could also be a result of image limitations. The galaxy exhibits a color gradient, with the central region appearing more yellow/white, indicating an older stellar population, transitioning to bluer hues in the outer regions, possibly due to younger stars and/or ongoing, though subdued, star formation. There is no clear evidence of spiral arm structure or a well-defined disk component. Minor asymmetry is noted, but this does not suggest a recent major merger event. The overall appearance suggests a galaxy in a relatively quiescent state.
