The galaxy appears to be a relatively smooth, elliptical galaxy with a slight elongation. It exhibits a concentration of light toward the center, suggesting a prominent galactic nucleus. There is a general lack of distinct spiral arm structures. The galaxy presents a yellowish hue, indicative of an older stellar population with fewer young, hot, blue stars. The shape appears to be somewhere between round and cigar-shaped. There are no obvious signs of major mergers or significant tidal disturbances affecting the galaxy's overall structure. There is a hint of bluer regions that could indicate areas of active star formation.
