The galaxy presents as a slightly elongated, disk-shaped structure. The central region exhibits a bright, concentrated core, suggesting a significant concentration of stars. The overall color profile is largely dominated by a blue-white hue, particularly in the central region, potentially indicating the presence of younger, hotter stars and ongoing star formation. However, there appear to be subtle color variations within the disk, with a hint of redder tones in some areas, possibly due to older stellar populations or dust obscuration. There is a possible sign of minor disruption, suggesting tidal interactions or a recent merger event. The disk appears relatively smooth, with no obvious spiral arm structures discernible in this image resolution. The galaxy has an estimated effective radius of just over 4 kiloparsecs.
