The galaxy appears to be a spiral galaxy, viewed at a significant angle relative to its disk plane, causing it to appear elongated, almost cigar-shaped. The central bulge is prominent and appears to be relatively smooth and concentrated, exhibiting a yellowish hue, suggesting an older stellar population. Faint spiral arms are visible extending from the central bulge, traced by regions of bluer light, possibly indicating the presence of younger, hotter stars and star-forming regions. These arms do not exhibit sharp definition. There is no obvious active galactic nucleus. There are no clear signs of major mergers or tidal disturbances.
