The galaxy presents as an elongated, cigar-shaped object. It appears to have a smooth morphology, lacking distinct spiral arms or a prominent bulge. The central region exhibits a slightly yellowish hue, potentially indicating an older stellar population and/or dust obscuration. Fainter, blueish light extends outwards from the central region, possibly denoting regions of more recent, but suppressed, star formation. There may be minor gravitational disturbances, but these are not significant enough to suggest a major merger event. The galaxy appears relatively isolated within the observed field.
