The galaxy presents as an elongated, disk-like structure, observed at an inclined angle relative to our line of sight. The central bulge appears prominent and exhibits a yellowish-orange hue, indicative of an older stellar population likely dominated by evolved stars. Moving outwards from the bulge, the disk becomes bluer in color, suggesting the presence of younger, hotter stars and ongoing star formation regions. The light is not evenly distributed throughout, and some areas of the disk are brighter than others. There is evidence of minor disturbances at the lower end of the disk, indicating a possible interaction with another galaxy or recent minor merger event. The overall morphology points towards a spiral galaxy with a relatively smooth texture, but also exhibiting features associated with disturbed systems.
