The galaxy presents as a relatively smooth, centrally concentrated object with a generally elliptical morphology. The core region exhibits a bright, yellowish hue, potentially indicative of an older stellar population dominating this area. Moving outwards from the center, the galaxy's light gradually fades into a more diffuse halo. There is minimal evidence of strong spiral arm structures or significant dust lanes within the visible light spectrum. The overall color profile suggests a lack of significant ongoing, active star formation, although the galaxy is still forming some stars, but at a relatively low rate. There is no readily apparent indication of any major merger events or strong tidal disturbances in its immediate vicinity, though some minor irregularities may exist upon closer inspection.
