The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge that appears yellow-white. This suggests an older stellar population, indicative of reduced recent star formation. The outer regions show a subtle decrease in surface brightness, fading into the background sky. There may be a hint of a disk-like component viewed at an angle, but the overall structure appears dominated by its spheroidal morphology. There's a slight elongation to the galaxy's shape, leaning more towards a spheroid with a cigar-like shape, as opposed to perfectly round, which might suggest it has experienced a recent, but not major, gravitational interaction.
