The galaxy presents as an elliptical or lenticular type, exhibiting a smooth and relatively featureless morphology. The light distribution is concentrated towards the center, forming a bright, prominent bulge region. This central region displays a yellowish hue, potentially indicating an older stellar population and reduced ongoing star formation. The outer regions of the galaxy appear fainter, suggesting a gradual decrease in stellar density with increasing radial distance. There is no discernible spiral arm structure, and the overall shape is somewhat rounded, though a slight elongation is detectable along one axis. Evidence of any significant tidal interactions or recent mergers appears minimal; however, there might be some minor disturbances in the outer regions. The galaxy's color gradient suggests a general trend from older, redder stars in the central bulge to slightly younger, bluer stars in the outer regions, though overall star formation appears subdued throughout the system.
