The galaxy presents as a moderately bright, elliptical or lenticular system. The light profile appears smooth, with a centrally concentrated bulge that is surrounded by a fainter and more diffuse halo. There is little evidence of distinct spiral arms or strong dust lanes. The overall color is predominantly yellow-red, suggesting an older stellar population with minimal ongoing star formation. A very slight asymmetry or subtle disturbance in the outer regions is visible, but the system is not actively merging. Overall, the galaxy exhibits a relaxed morphology, indicative of a relatively evolved system that is no longer actively assembling or undergoing major interactions.
