This galaxy appears to be a spiral galaxy, seen edge-on from our vantage point. A prominent central bulge is observed, with a relatively smooth and diffuse light profile, indicating a significant population of older stars. A flattened disk structure extends outwards from the bulge. Within the disk, we see a faint, bluish hue which suggest the presence of younger, hotter stars and ongoing star formation. There is no strong evidence of a major merger or tidal disturbance. It is difficult to see if it has defined spiral arms based on the edge on perspective, but the disk itself appears to be relatively undisturbed.
