The galaxy appears as an elongated, disk-shaped structure, presenting an edge-on orientation relative to our line of sight. A prominent central bulge is visible, characterized by a reddish hue, suggesting a population of older stars. The disk shows a mix of colors, with greenish regions indicating areas of active star formation. There appears to be a relatively smooth distribution of light throughout the galaxy, with no clear spiral arm structure visible. The galaxy's morphology indicates a late-type disk galaxy with a substantial bulge. There appears to be no major merging events, and there are no major disturbances in the structure of this galaxy. 
