The galaxy presents as a relatively smooth, disk-shaped structure. Its form is elongated with a high ellipticity, suggesting an edge-on or nearly edge-on orientation relative to our line of sight. The central bulge exhibits a bright, concentrated luminosity, appearing yellowish. The disk component displays a color gradient, transitioning from a yellowish hue near the central bulge to bluish tones at the outer edges, possibly indicating regions of more recent star formation in these areas. There may be some minor disturbances to the main galaxy from small interactions, however the image is not clear enough to confirm any interaction.
