The galaxy presents a generally elliptical morphology, exhibiting a smooth light distribution without prominent spiral arms or a distinct bar structure. The central region displays a concentrated luminosity, appearing significantly brighter than the surrounding areas. The color profile suggests a redder core, transitioning to slightly bluer hues in the outer regions. There may be some minor structural asymmetries, which could indicate past or ongoing interactions, but no major disturbances are visible. The overall appearance is consistent with a relatively evolved galaxy, potentially an elliptical or lenticular type, located at a considerable distance.
