The galaxy appears to be a disk galaxy viewed at a high inclination, nearly edge-on. It exhibits a relatively smooth appearance, with a bulge that occupies roughly 50% of the galaxy. Faint spiral arms are potentially present but hard to see, with the disk gradually fading at the edges. There is no strong evidence of ongoing major mergers or significant tidal disturbances; minor disturbances cannot be ruled out. The galaxy has a moderately cigar-like shape. The light distribution suggests the galaxy is dominated by an older stellar population with only some small regions of star formation, primarily concentrated within the disk. Overall, this galaxy is of moderate luminosity and mass, with a correspondingly moderate rate of star formation.