The galaxy presents as a relatively smooth, elongated structure. Its shape is cigar-like, with an apparent lack of distinct spiral arms. There is a concentrated central bulge with a yellowish hue, suggesting an older stellar population. Surrounding the bulge is a fainter, more diffuse disk. The overall color gradient suggests a transition from older stars in the center to slightly younger stars in the outer regions. The galaxy displays no signs of major ongoing mergers or strong tidal disturbances, but there are some slight irregularities in the outer disk.