The galaxy presents as a moderately luminous object, appearing relatively smooth in overall structure with a somewhat elliptical morphology. The central region exhibits a pronounced concentration of light, suggesting a prominent bulge component potentially comprised of older stellar populations. Moving outward from the core, the light intensity decreases, transitioning into a more diffuse halo. There is a subtle color gradient visible, shifting from slightly redder hues in the central bulge to subtly bluer tones within the surrounding regions. This could be indicative of ongoing, albeit moderate, star formation within the outer regions of the galaxy. Indications of a possible minor merger event with a small irregular extension of the galaxy.
