The galaxy presents a generally smooth and rounded morphology, appearing largely featureless upon initial inspection. The primary light distribution suggests an elliptical or lenticular classification. The color profile indicates a population of older stars with an absence of significant ongoing star formation. The slight asymmetry in the light distribution and presence of a faint tidal tail suggests a possible past minor interaction or merger, however this feature is subdued. The object is relatively compact, with a dense central concentration of light. 
