The galaxy presents a generally smooth appearance with a dominant central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population.  The overall shape is more rounded than elongated, though not perfectly spherical.  There may be some hints of a very faint disk component surrounding the bulge, but this is difficult to ascertain definitively from the image due to limited resolution. There is no obvious evidence of strong spiral arm structure or significant tidal disturbances suggesting recent major mergers or interactions.  The galaxy appears relatively undisturbed.
