The galaxy presents as a well-defined, elongated elliptical shape. It exhibits a relatively smooth morphology, lacking any obvious spiral arm structures or prominent dust lanes. The central region appears brighter and more concentrated, suggesting a dense nucleus. The color profile suggests a possible gradient, transitioning from a slightly bluer hue in the outer regions to a redder tone towards the core. This color variation might indicate a differential stellar population, with younger, bluer stars populating the outskirts and older, redder stars concentrated in the center. There are no immediately apparent signs of ongoing major mergers or tidal disturbances; however, the image resolution limits the detection of subtle features.
