The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth, featureless morphology. It is centrally concentrated with a bright core. The shape tends to lean towards a "in between" rounded shape, but is not perfectly circular. There is no clear evidence of spiral arms or a prominent disk structure within the available image resolution. The color profile suggests a mature stellar population, as the galaxy is largely redder in hue. There is no apparent presence of any major ongoing merging activity, but potential minor disturbance or interaction may be subtle. Overall, this galaxy presents as a relatively evolved system.
