The galaxy presents a generally smooth morphology, appearing largely featureless. It exhibits a roughly circular or slightly elliptical shape. The light distribution appears concentrated towards the center, but with a gradual decline in intensity outwards. There is a hint of a possible disk structure, but it is not clearly defined or prominent. No obvious spiral arms or bar-like structures are apparent. There are no signs of any major disturbances from recent mergers or interactions and appears to be generally isolated. The color is slightly redder, indicating a potentially older stellar population and a relatively low rate of current star formation.
