The galaxy presents an elongated, cigar-shaped morphology. The central region exhibits a concentration of yellow-white light, indicative of an older stellar population. This core gradually fades into the outer regions. There appears to be a faint blue region at one end of the galaxy, suggesting the presence of younger, hotter stars and potentially ongoing star formation. The overall structure suggests a relatively smooth distribution of light, with minimal signs of spiral arms or significant dust lanes. There is some minor visual disturbance along the galaxy that could be a sign of tidal interactions.
