The galaxy presents a morphology consistent with an elliptical or lenticular type. Its overall structure appears relatively smooth, with a central bulge that seems to dominate the light profile. The luminosity concentration is high in the center, suggesting an older stellar population. There is a faint, diffuse halo surrounding the central region, gradually fading into the background. The galaxy exhibits a slight flattening and ellipticity, with an apparent major axis orientation. There's a subtle color gradient visible, with the central bulge having a more reddish or yellowish tint, potentially indicating a higher concentration of older, cooler stars and dust, in contrast to the outer regions, which exhibit a bluer hue, implying a younger stellar population. No prominent spiral arms or obvious dust lanes are discernible.
