The galaxy presents as an elongated, disk-shaped structure, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue that suggests an older stellar population. The disk itself appears relatively smooth, lacking strong evidence of distinct spiral arms. There is a slight bluer tint to the disk compared to the central bulge, potentially indicating the presence of younger stars and ongoing star formation, albeit at a modest rate. The galaxy does not show any obvious signs of interaction or recent merger events. There is a red region in the image that could show dust.
