The observed galaxy presents as a moderately bright, disk-shaped system, with a noticeable bulge. Its orientation is close to edge-on relative to our line of sight. The central bulge exhibits a yellowish hue, possibly indicating an older stellar population. Fainter and bluer regions are visible extending outwards from the bulge on either side, suggesting the presence of younger stars. Additionally, there is evidence of internal disturbances. Patches of irregular dust and/or gas are present, with some indicating a potential merging event or tidal interaction, particularly at the lower side of the galaxy.
