The galaxy presents a primarily smooth morphology, with a somewhat elliptical shape. A central bulge is readily apparent, exhibiting a high surface brightness and a yellowish-white color, suggesting an older stellar population. Fainter, more diffuse light extends outward from the bulge, forming a halo. There may be some irregularities in the outer regions. These irregularities suggest the presence of either tidal disturbances, perhaps caused by a minor merger, or faint spiral structures. Overall, the galaxy is relatively compact, but the classification is difficult based on the image alone. Further spectroscopic data is needed for a more complete description.
