The galaxy presents as a relatively bright, centrally concentrated object. It appears to have a somewhat diffuse morphology, transitioning from a high surface brightness core to a fainter, less distinct outer region. There is a subtle, disk-like component but is more clearly an elliptical galaxy. No clear spiral arm structures are discernible. Color gradients exist within the galaxy; the core exhibits a yellower hue, suggestive of an older stellar population, while the outer regions have a bluer tint. There is some clumpy structure within the galaxy, which could be a consequence of ongoing star formation. The image indicates that the galaxy does not seem to be undergoing any major interaction or merging events.
