The galaxy presents as a relatively smooth, elliptical-like system. It has a concentrated, bright central bulge that transitions gradually outward to a fainter, more diffuse halo. The core exhibits a yellowish-orange hue, which likely indicates an older stellar population. There is a notable absence of distinct spiral arms or prominent dust lanes. The overall shape appears nearly circular, exhibiting minimal ellipticity. There is no visual indication of significant tidal disturbances or ongoing major mergers. Subtle color variations are present, suggesting varying ages and metallicities within the stellar population. There appears to be little active star formation, based on the lack of blueish clusters or nebulae within the visible spectrum.
