The galaxy exhibits a generally smooth morphology with a central concentration of light. The object appears largely spheroidal in shape, with an apparent lack of defined spiral arms or a prominent disk structure. A slight elongation is discernable, deviating from a perfectly circular profile. The color gradient suggests an older stellar population, with a yellowish hue dominating the central region. The outer regions show a subtle color shift towards redder wavelengths. There is no visually apparent ongoing major merger activity or significant tidal disturbances.
