The galaxy presents as a relatively small, elongated object with a clear disk morphology, observed nearly edge-on from our vantage point. A prominent central bulge is visible, appearing somewhat rounded, although some structure may be obscured by the angle of observation. The galactic disk exhibits a color gradient, appearing bluer at the lower extent, potentially indicating regions of more active star formation, and redder tones extending upward from the central bulge. There may be a presence of slight disturbance within the disk, perhaps from a minor interaction, however it is difficult to determine at this resolution. The galaxy does not appear to be undergoing a major merger. The smooth overall appearance with an edge on disk suggest a high likelihood that this is a spiral galaxy.
