The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated core with a yellowish-white hue, suggesting an older stellar population. A fainter, more diffuse reddish halo extends outwards from the core, potentially indicating the presence of dust or a slightly younger stellar population in the outer regions. Overall, the galaxy shows little evidence of significant star formation. No spiral arms or distinct morphological features are readily apparent, suggesting that it is a relatively quiescent system. There is no obvious indication of any current or recent major merger activity. The light distribution appears relatively even, with only minor irregularities.
