The galaxy presents as an elliptical morphology with a high degree of central concentration and an axial ratio around 0.8, suggesting it is likely a flattened Elliptical or S0 type galaxy. There is a bright central bulge with evidence of a smoothly distributed stellar population. The galaxy appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal features. Faint disk or spiral arm features are indistinct. The galaxy's color is noticeably redder in the central bulge, indicating an older stellar population, with bluer hues in the outer regions implying more recent star formation. The object is well-defined, and the smooth profile indicates that the system is relatively relaxed.
