The galaxy presents a generally smooth appearance, lacking prominent spiral arms or a well-defined bar structure. Its overall form is somewhat elliptical, exhibiting a moderate degree of roundness. There is no evidence of ongoing major mergers or significant tidal disturbances; the galaxy appears relatively undisturbed. A central bulge is discernible, with the light gradually fading outwards from the core. The color profile suggests a population of older stars, with a redder overall hue.
