The galaxy presents a largely smooth morphology. It appears elliptical in shape, with a somewhat elongated form. The central region exhibits a bright, concentrated core of light, suggesting a high stellar density or possible active galactic nucleus. The color distribution is relatively uniform, with a slight blue tint. This hue might indicate moderate levels of recent star formation, although the overall smoothness implies that the galaxy is primarily composed of an older stellar population. There is a slight suggestion of a minor disturbance or tidal feature on one side, which could be indicative of a past or ongoing minor merger event.
