The galaxy presents as an elongated structure, appearing somewhat cigar-shaped. There is a notable concentration of light towards the central region, suggesting a bulge. The color profile indicates a higher concentration of redder wavelengths along the major axis of the galaxy, potentially indicating older stellar populations or dust obscuration. There appears to be a possible tidal feature or disturbed morphology on one end, indicating a possible gravitational interaction or merger event. The galaxy overall appears to be relatively smooth. There appears to be a high amount of dust or aging stars as very little blue light is observed from the galaxy.
