The observed galaxy presents an elliptical morphology, elongated along a principal axis, with an approximate axis ratio of 0.5. A smooth, diffuse light profile dominates the galaxy's structure, suggesting a relatively old stellar population and minimal ongoing star formation. The color gradient transitions from a yellowish central region to a redder outer halo, indicative of metallicity variations or differential stellar ages within the galaxy. No distinct spiral arms or dust lanes are discernible. The galaxy appears relatively undisturbed, lacking any signs of recent merger activity or tidal features. The overall impression is that of a mature, early-type galaxy.
