The galaxy presents a diffuse morphology, displaying a central region of increased luminosity. While a distinct spiral structure is not readily apparent, the overall form suggests a flattened disk-like structure viewed at a moderate inclination. Blue hues are noticeable, particularly in the outer regions, suggesting the presence of younger, hotter stellar populations associated with ongoing or recent star formation. There is also a hint of redder hues, perhaps due to older stellar populations or the presence of dust. The light distribution appears somewhat disturbed, possibly indicative of past or ongoing interactions with another galaxy. Faint tidal tails or disrupted features are not obvious, but the irregularity suggests the presence of a minor disturbance or recent merger. The central bulge appears relatively small compared to the overall size of the disk, suggesting a late-type spiral or irregular galaxy classification.
