The galaxy appears to be a relatively smooth, elongated structure. The central region exhibits a bright, diffuse glow with a yellowish hue, suggesting an older stellar population. The galaxy's shape is somewhat cigar-like, more elongated than circular, but not a thin disk. There is a hint of a fainter, more diffuse halo surrounding the central region. There are no obvious spiral arm structures, but a slight bluer tinge near what may be the edge of the structure suggests possible recent star formation in that area. There is no apparent strong evidence of a recent major merger or significant tidal disturbances, but minor irregularities in its shape or faint extensions cannot be entirely ruled out given the resolution.
