The galaxy presents a generally smooth, elliptical morphology. There is a high degree of central concentration, with a bright, unresolved core suggesting the presence of an active galactic nucleus or a dense stellar population. The overall color appears somewhat blueish, indicating the presence of a moderate population of relatively young, hot stars, but it is dominated by a generally older population. The outer regions of the galaxy fade smoothly into the background, suggesting a lack of significant tidal interactions or recent major mergers. No prominent spiral arms or significant dust lanes are readily apparent. There is no obvious sign of a strong ongoing merger event, but there may be some minor disturbance in the galaxy's outer regions. The galaxy exhibits a nearly circular appearance.
