The galaxy appears to be a spiral type, observed at a significant angle relative to our line of sight, indicating a disk orientation approaching edge-on. While specific spiral arm structures are difficult to resolve given the viewing angle and image resolution, there is a noticeable elongation and asymmetry in the distribution of light, suggesting the presence of arms and possibly a weak bar feature. A prominent central bulge is visible, exhibiting a concentrated luminosity. The color profile suggests a mix of stellar populations, with a yellower hue in the bulge possibly indicating older, redder stars and lower dust content, while the outer disk shows bluer, more actively star-forming regions. Overall, the galaxy presents a fairly organized structure, with no major morphological disturbances evident from its appearance, but subtle irregularities indicate possible past interactions or mergers.
