The galaxy presents as a relatively smooth object, with a somewhat elliptical morphology. The central region exhibits a higher surface brightness, indicative of a concentrated core. A slight flattening is observed, deviating from a perfect spherical shape. Color gradients are subtle, with a tendency toward bluer hues in the outer regions and a more uniform coloration in the inner regions. This suggests a relatively homogenous stellar population or dust distribution within the central region. The galaxy lacks prominent spiral arm structures or distinct features typically associated with active star formation regions. The overall appearance suggests a galaxy nearing a transition from a star-forming to a quiescent state, dominated by an older stellar population.
