The galaxy presents as a somewhat elliptical or lenticular structure, appearing more elongated than perfectly spherical. There is a smooth, centrally concentrated light distribution, with no apparent spiral arm structures. A prominent bulge is visible, brighter and more condensed than the outer regions. There is an indication of a faint disc extending beyond the bulge, but its features are indistinct. The galaxy has a slight color gradient; its core and bulge are dominated by yellow and white hues, with the outer regions trending slightly blue, suggesting the presence of a population of younger, hotter stars. Overall, the galaxy appears relatively undisturbed and likely quiescent in terms of major star formation activity. There is possible evidence of a minor interaction or disturbance in the galaxy shape.
