The galaxy presents an elongated, somewhat cigar-shaped morphology. There is a notable color gradient across its structure. A central, reddish core is observed, suggesting an older stellar population likely dominating the region. Extending outwards from this core, bluer hues become more prominent, suggesting the presence of younger, hotter stars, particularly in the outer regions or possibly within a disk-like component. The overall appearance indicates that this galaxy is likely a spiral galaxy, with signs of a slight disturbance or possibly some tidal features present. There is an uneven surface brightness distribution, implying the system may be dynamically active, or that it has experienced a recent interaction. There may be active star formation occurring, as supported by the blue coloration in the galaxy, and a relatively high stellar mass.
