The galaxy presents an elongated, cigar-shaped morphology. A prominent central bulge dominates the structure, exhibiting a smooth, diffuse light profile, suggesting an older stellar population. A disk component is subtly discernible, oriented approximately diagonally across the image. The disk appears somewhat disturbed, with hints of asymmetry and faint, irregular features possibly indicating minor tidal interactions or internal instabilities. Color gradients suggest the presence of ongoing, but potentially limited, star formation within the disk, contrasting with the redder bulge. There is no clear evidence of a major merger, though some subtle disturbances are visible. The overall appearance suggests a transitional object, possibly evolving from a spiral towards an elliptical morphology.
