This galaxy presents a primarily smooth, elliptical morphology. It exhibits a notable central bulge that appears nearly spherical. The color gradient suggests a relatively older stellar population dominating the core, indicated by the yellowish-orange hue. Fainter, bluer colors are observed towards the outer edges of the galaxy, which may indicate regions of more recent, albeit limited, star formation activity. The galaxy displays a slight elongation, with the "in between" classification being the most noticeable. There are no strong indications of spiral arm structures or prominent dust lanes. No major merger events were detected. Small hints of minor disturbances are detected, but further observation is needed to say for certain.
