The observed galaxy presents as an edge-on spiral. A prominent disk structure is evident, appearing relatively smooth with faint features. The bulge is not significantly pronounced; it appears subtle and elongated along the disk. The dust lane is not clearly visible. The overall colour of the galaxy leans towards the redder end of the spectrum, indicating a population of older stars and a relatively low star formation rate. The morphology suggests the galaxy is relatively isolated and undisturbed. There are no obvious signs of interactions with other galaxies, or of a recent major merger event. The size of the galaxy appears typical for spiral galaxies.
