This galaxy presents as an elliptical-like system, exhibiting a centrally concentrated luminosity profile. The core displays a bright, yellowish-white color, suggesting a concentration of older stellar populations. The galaxy appears to be moderately flattened with its overall shape tending towards an intermediate elliptical classification. Faint, diffuse bluer light extending outward from the central bulge may suggest some residual star formation activity, however the overall smoothness of the light distribution indicates that this galaxy is not a spiral. The galaxy appears relatively undisturbed with no major signs of ongoing merger activity or significant tidal distortions.
