The galaxy presents a generally smooth morphology, with a spheroidal shape. There is a distinct central bulge, which appears to be the brightest region of the galaxy and exhibits a yellowish hue. The light intensity decreases gradually from the center outward, without any sharp boundaries or distinct spiral arm structures visible. The overall color profile suggests a relatively old stellar population. There are no clear indications of active galactic nuclei (AGN) activity or significant dust lanes. Faint diffuse light extends from the central region, giving the galaxy a relatively large apparent size. There are no obvious signs of any ongoing major merger events or tidal disturbances.
