The galaxy presents as a relatively smooth, somewhat elliptical structure. The light distribution appears centrally concentrated with a yellowish core, suggesting an older stellar population dominating the central regions. Fainter, bluer regions are visible surrounding the core, indicating the presence of younger stars, possibly within faint spiral arm structures or disk components. Overall, there is no strong indication of major disturbances or ongoing major mergers, although the overall color profile does indicate some ongoing star formation. The galaxy's overall shape is more elliptical than disk-like.
