The galaxy presents as a somewhat smooth, elongated structure. Its overall shape is notably cigar-shaped, with a high aspect ratio. The central region is brighter and exhibits a yellowish hue, which might indicate a higher concentration of older stellar populations. The outer regions appear fainter and display a slightly bluer tint, which could signify the presence of younger, hotter stars or ongoing star formation. The galaxy does not appear to be undergoing any major merging events, although minor disturbances cannot be ruled out.
