The galaxy presents a largely smooth and rounded morphology, characteristic of an elliptical or lenticular galaxy. Its central bulge is luminous, displaying a yellowish-white hue, potentially indicating an older stellar population. The light distribution decreases gradually towards the outer regions. Faint blue tinges are visible in the outer disk, suggesting the presence of some younger, hotter stars, although star formation appears relatively subdued. There is no evidence of prominent spiral arms or a distinct dust lane. The overall structure is fairly undisturbed, showing no significant signs of tidal interactions or recent merger events.
