The galaxy presents as a disk-like structure, viewed edge-on or at a highly inclined angle to our line of sight. Its morphology appears relatively smooth, suggesting a possible early-type spiral or lenticular classification. A central bulge is evident, displaying a yellowish-red hue, possibly indicating an older stellar population. Fainter, bluish regions are observed within the disk, suggesting the presence of younger stars and ongoing star formation. The overall shape is elongated, with a cigar-shaped appearance. There is no prominent evidence of major mergers or tidal disturbances in the immediate vicinity.
