The galaxy presents a distinct elongated morphology, appearing as a cigar shape on the plane of observation. Its light profile suggests a relatively smooth distribution of stars and gas, with a subtle hint of a central concentration. The galaxy appears reddish in color, indicating an older stellar population with likely ongoing star formation. There may be minor disturbances as the galaxy shows signs of potential interactions with other galaxies, with a possible asymmetry in its overall structure. The galaxy appears to be relatively isolated with no clear evidence of major mergers.
