The galaxy presents a generally smooth and elliptical morphology, appearing largely featureless without prominent spiral arms or a defined disk structure. The light distribution exhibits a concentration towards the center, suggesting a dense galactic nucleus. The overall color appears to be on the redder end of the spectrum, indicative of an older stellar population with a lower rate of ongoing star formation. While appearing mostly undisturbed, there may be some minor tidal features, yet no major signs of ongoing merger activity.
