The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its overall color appears yellowish-orange, suggesting a stellar population dominated by older, redder stars. There is a subtle color gradient visible, with the central region exhibiting a more pronounced yellow hue compared to the slightly redder and more diffuse outer regions. The shape is nearly circular on the plane of observation, with a slight extension that may be indicative of a weak disc structure viewed nearly face-on. There are no visually apparent spiral arms or significant dust lanes, lending further support to the classification of this galaxy being an early type system. Any subtle irregularities in the outer envelope suggest possible minor disturbances, such as a past minor merger.
