The galaxy presents a generally smooth and rounded morphology. There is no obvious spiral arm structure or central bar. The object appears as a concentrated, single entity rather than showing any signs of merging activity or significant tidal disturbances. The color profile exhibits a central concentration of yellow light that fades into redder hues at the edges, suggesting an older stellar population with minimal ongoing star formation. The light distribution is centrally concentrated, decreasing steadily outward from the core. The object exhibits characteristics consistent with an elliptical galaxy or a lenticular galaxy with a dominant bulge component.
