The galaxy presents a generally smooth morphology, appearing as a diffuse, elongated structure. There is a central concentration of light that brightens into a central region, suggesting a bulge component. The color appears somewhat redder in the galaxy's central part, possibly indicating an older stellar population, with the outer regions exhibiting a bluer tinge. No obvious spiral arms or distinct features are observed, but the galaxy does show some minor disturbance, possibly indicating the presence of recent or ongoing interactions. Overall, the galaxy presents a relatively undisturbed structure, consistent with a galaxy that has completed the majority of its evolution.
