The galaxy presents an elongated, cigar-shaped morphology. Its light distribution appears relatively smooth, lacking any distinct spiral arm structures or prominent knots of star formation visible at this resolution. The color gradient suggests a slightly bluer core region transitioning to redder hues towards the outer edges, potentially indicating a decline in ongoing star formation further from the galactic center. There may be some evidence of minor gravitational disturbances, such as subtle distortions, but no large-scale tidal features or clear signs of major mergers are apparent. The galaxy is neither particularly compact nor highly diffuse, and the light profile suggests a centrally concentrated mass distribution.
