The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. It appears as a flattened ellipsoid, with a major axis significantly longer than its minor axis. The color gradient transitions from a yellowish-orange core to a fainter, greenish-blue outer region. This may indicate an older stellar population towards the center and younger, star-forming regions in the disk. There is no strong evidence of spiral arms or a bar structure. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances, though very minor disturbances cannot be ruled out at this resolution. The overall light distribution is relatively even, suggesting a well-mixed stellar population.
