The galaxy presents a predominantly smooth appearance, with a noticeable elongation along its major axis, exhibiting a cigar-like shape. A central bulge is visible, exhibiting a yellowish hue, suggesting an older stellar population. The disk component appears relatively thin and faint, displaying a bluish tint, indicative of ongoing star formation. Faint spiral arm structures might be present, but their visibility is limited. There is evidence of some disturbance in the disk, possibly resulting from minor gravitational interactions or internal dynamics. Overall, the galaxy appears to be a disk galaxy, likely seen edge-on, experiencing a moderate level of star formation.
