The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge that gradually diffuses outwards. Its color profile suggests an older stellar population, with a dominant yellow-red hue, indicative of evolved stars and a diminished rate of active star formation. There is no apparent spiral structure or significant dust lanes visible. The galaxy presents a regular, rounded shape, lacking any major morphological disturbances or signs of ongoing mergers, though minor disturbances cannot be ruled out. It is not perfectly circular but appears as if in between circular and cigar-shaped.
