The galaxy presents as a moderately bright, disk-shaped system, viewed at an intermediate angle, not quite edge-on, but with noticeable flattening. Its light is concentrated towards the center. The core region exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions of the disk are less well-defined, appearing fainter and exhibiting a slightly bluer tint, suggesting the presence of some younger stars. There's a possible hint of spiral structure but it is not very pronounced. The galaxy appears relatively isolated with no obvious signs of major disturbances or mergers. It seems like a relatively massive galaxy with a low star formation rate.
