This galaxy exhibits a morphology suggestive of a disk galaxy viewed at a significant inclination angle. The central bulge region appears relatively bright and compact, with a bluish hue indicating the presence of hot, young stars. Extending outward from the bulge, a fainter disk structure can be discerned, with a color gradient shifting towards redder hues, implying a population of older stars and/or dust obscuration. The galaxy's overall shape is elongated, consistent with an edge-on or highly inclined disk. Subtle irregularities in the disk's structure may indicate minor gravitational interactions or internal dynamical processes. Although the disk appears relatively smooth, a slight asymmetry in the distribution of light could suggest a subtle disturbance. The galaxy displays evidence of active star formation, inferred from its blue color and considerable absolute magnitude. The galaxy demonstrates moderate mass and star formation rates. 
