The galaxy presents as a generally smooth and elongated structure. There is a significant central bulge exhibiting a yellowish hue, suggesting an older stellar population in this region. Extending outward from the bulge is a disk component, though it appears relatively faint and less defined. The overall color of the disk seems bluer than the central bulge, possibly indicating the presence of younger, hotter stars and ongoing star formation. The galaxy exhibits a noticeable cigar shape. There is no obvious evidence of strong spiral arm structure or major disturbances. There is also little indication of a significant merger event or tidal interactions with other galaxies.
