The galaxy presents as a relatively smooth, disk-shaped structure viewed nearly edge-on. A distinct dust lane bisects the galaxy, obscuring the central bulge region. The galaxy appears elongated, with a length approximately twice its width. There is a slight asymmetry to the outer disk, potentially indicative of tidal interactions or past merger events. Faint, diffuse extensions are visible beyond the main disk, suggesting a possible halo or extended stellar population. The color profile suggests a mix of stellar populations, with bluer hues at the edges, suggestive of recent star formation, and redder hues in the central bulge, indicating an older population. Based on the overall morphology and color distribution, this galaxy appears to be an intermediately massive spiral or lenticular galaxy with a modest degree of star formation. There are no obvious signs of a major ongoing merger, however there may be signs of minor disturbances.
