The galaxy presents as a centrally concentrated object with a generally smooth morphology. Its overall shape approximates an elliptical form, exhibiting a moderate degree of ellipticity. A distinct bulge is observed in the central region, characterized by a yellowish-white hue, potentially indicating an older stellar population. The surrounding halo appears fainter, with a subtle bluish tint. This suggests the presence of a younger stellar population with ongoing star formation at a low rate within the outer regions. No distinct spiral arm structures or prominent dust lanes are discernible. There is no clear indication of any major mergers or significant tidal disturbances affecting the galaxy's overall structure, though minor disturbances cannot be ruled out.
