The galaxy presents a generally smooth morphology, suggesting it is likely an elliptical or lenticular galaxy. The central bulge is well-defined and exhibits a yellowish hue, consistent with an older stellar population. The galaxy appears somewhat elongated rather than perfectly circular, but not highly elongated. There is some indication of a faint, diffuse disk component surrounding the bulge. Overall, the galaxy displays a settled appearance with no obvious signs of major mergers or significant tidal disturbances, although there may be some minor asymmetry.
