The galaxy presents as a largely smooth, elliptical-like structure. There is a dominant, centrally concentrated luminosity, suggesting a substantial bulge component. The galaxy's color profile exhibits a yellowish hue in the center, possibly indicating an older stellar population. Moving outward from the center, there is a gradual shift toward bluer colors, implying the potential presence of younger stars or ongoing star formation activity in the outer regions, although this appears subdued. Overall, the galaxy lacks prominent spiral arms or other distinct features, and appears largely undisturbed.
