The galaxy presents as a roughly elliptical, though not perfectly circular, structure with a smooth overall appearance. The central region exhibits a concentrated luminosity, appearing more yellow, perhaps indicative of an older stellar population. Fainter, bluer light extends outward from the central bulge, suggesting some presence of younger stars and possibly ongoing star formation, though not at a rate high enough to disrupt the overall smooth morphology. There's a slight indication of a disk-like component with a minor degree of disturbance. This could be due to a previous minor merger event, or it could be an internal structural feature. There is no clear sign of prominent spiral arms or a strong bar structure. Based on the observed color gradients and lack of significant morphological disturbances, the galaxy may be transitioning from a more active, star-forming phase to a more quiescent state.
