The galaxy presents an overall smooth morphology. It exhibits an elongated, cigar-shaped structure. The central region is dominated by a bright, yellowish core, suggesting a concentration of older stellar populations. Fainter, bluer hues are visible in the outer regions of the galaxy, particularly extending along the major axis. The blue color may indicate the presence of younger, hotter stars and ongoing star formation. However, the overall smoothness suggests that the galaxy is likely an early-type spiral or lenticular galaxy viewed at an angle. There is no obvious evidence of major mergers or tidal disturbances, only a small disturbance.
