The galaxy appears as a centrally concentrated object, exhibiting a largely smooth morphology. The light distribution suggests a near-spherical shape. There are no apparent spiral arms or strong dust lanes visible. A faint, extended halo may be present, but the signal is weak and difficult to discern. Based on the color profile, which is brighter in the center, there may be little to no current star formation. There is no visible evidence of any major mergers or tidal disturbances impacting the galaxy's structure.
