The galaxy presents as a moderately luminous, elongated structure. It exhibits a central bulge that is roughly spherical, appearing smooth and densely packed, with a color suggesting an older stellar population. Extending outward from the central bulge is a disk, also appearing smooth, but with a bluer hue indicating the presence of younger, hotter stars or star-forming regions. The disk's light is fainter than the bulge, and its shape is more cigar-like. No distinct spiral arm structure is discernible. There is no apparent interaction with any other galaxies or signs of significant tidal disturbances.
