The galaxy presents an elongated, cigar-like morphology, suggesting a possible edge-on disk orientation. The central bulge appears brighter and exhibits a yellowish hue, indicative of an older stellar population. Fainter, bluish regions are visible within the disk, potentially signifying areas of ongoing star formation. There is a slight asymmetry or disturbance along one edge of the disk, warranting further investigation into possible minor interaction with another galaxy or internal dynamic processes. Overall, the galaxy appears relatively smooth, but shows hints of more complex underlying structures and potential activity.
