The galaxy appears as a relatively smooth, rounded structure. There is evidence of disturbed morphology, possibly indicative of minor gravitational interaction or a past merger event. The galaxy's light is mostly a yellow-orange color, but there is a faint red and slight blue tinge to some regions. The primary central region has a high concentration of light, indicative of either a bulge or a very bright core. The galaxy exhibits some irregularities in its shape, suggesting there might be tidal features or ongoing interaction affecting its overall structure. These irregularities appear in both the disk and halo of the galaxy. The outer edges of the galaxy gradually fade into the background, indicating a smooth stellar distribution.