The galaxy presents as a largely featureless elliptical type, exhibiting a smooth, centrally concentrated luminosity profile. The galaxy is elongated in shape, with the ratio of its major to minor axis suggesting a classification between E4 and E6 on the Hubble scale. The central bulge is prominent and appears to be composed of older stellar populations, indicated by its yellowish-orange hue. There is a slight color gradient, with the outer regions appearing bluer, perhaps indicating some ongoing or recent star formation, although this is not visually pronounced. No distinct spiral arms, dust lanes, or signs of active galactic nuclei activity are discernible in this image. There is no strong evidence of an ongoing or recent merger event, though subtle asymmetries cannot be ruled out at this resolution. The galaxy appears relatively isolated.
