The galaxy exhibits a clear disk-like morphology, viewed almost perfectly edge-on. The bulge appears prominent and exhibits a rounded structure. There is no clear evidence of spiral arm structures, likely due to the viewing angle, nor of any ongoing major merger activity or significant tidal disturbances. The colour of the galaxy appears to be moderately red, especially toward the central bulge. There is no indication of patchy dust lanes or significant star formation regions visible in this image. Based on its colour and overall morphology, the galaxy is likely dominated by an older stellar population, with relatively low recent star formation. There is very slight evidence of a boxy bulge. The galaxy appears to be relatively isolated.
