The galaxy presents as a moderately inclined, disk-shaped structure with a predominantly smooth appearance. The central region exhibits a slightly brighter, yellowish-white hue, suggesting a concentration of older stellar populations. Moving outward from the core, the disk transitions to a bluer color, indicating the presence of younger, hotter stars. The overall smooth texture suggests a lack of prominent spiral arm structures, but there appear to be subtle, elongated features suggestive of a disrupted disk. There is a slight warp or possible tidal distortion visible at the bottom of the galaxy. The galaxy appears relatively isolated.
