The galaxy presents as a moderately inclined disk galaxy, close to edge-on. The dust lane is prominent, bisecting the galaxy's bulge and obscuring a significant portion of the galactic plane. The color of the galaxy appears to show a gradient, with the central bulge region exhibiting a redder hue, suggesting an older stellar population. The outer edges of the disk show bluer colors, potentially indicating regions of active star formation. The overall morphology suggests the galaxy has a relatively smooth structure but may be undergoing some disturbances, potentially from a minor interaction. The shape is elongated, consistent with a spiral disk, and presents some irregularities.
