The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge.  The galaxy exhibits a yellowish hue, suggesting a population of older stars. There is some evidence of a faint disk structure surrounding the central bulge, although it is not well-defined and appears relatively featureless. There is no indication of strong star formation. The lack of defined spiral arms or prominent dust lanes further supports this classification.  The overall morphology suggests a galaxy that is not actively undergoing significant mergers or interactions with other galaxies.
