The galaxy presents as an edge-on spiral or lenticular system. A central bulge is prominent, exhibiting a yellowish-white hue, suggesting an older stellar population with less active star formation in that region. Fainter, bluer light extends along the galactic plane on either side of the bulge, indicating the presence of a disk component. This bluer color suggests the presence of younger, hotter stars and potentially ongoing star formation within the disk. There are no obvious signs of a bar structure or tidal features indicative of recent major mergers. Minor disturbances may be present within the disk, but require closer inspection to determine if they are real or artifacts. The galaxy appears relatively undisturbed and exhibits a generally smooth morphology. The size of the galaxy is not easily determined visually, but it appears to be a relatively large and massive system.
