The galaxy presents as a relatively faint, edge-on spiral. A distinct central bulge is visible, with a generally round morphology. The disk appears thin, with hints of dust lane absorption along the equatorial plane, although image resolution limits detailed analysis. Color gradients suggest a bluer stellar population in the outer disk compared to the redder bulge. No prominent spiral arm structures or active star-forming regions are discernible in this image. There are no obvious signs of tidal disturbances or ongoing mergers. Overall, this appears to be a relatively undisturbed, evolved spiral galaxy.
