The galaxy presents as a relatively smooth, elliptical-like structure with a central concentration of light. It appears to be primarily spheroidal with only a slight elongation. There are no obvious spiral arms or bar features visible. The central region exhibits a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy show a subtle gradient towards a bluer color, which could indicate the presence of a younger, star-forming population, though limited in extent. Overall, the galaxy appears largely undisturbed, showing no strong evidence of recent major mergers or tidal interactions. The morphology indicates a galaxy in a relatively quiescent state.
