The galaxy presents as a disk-shaped structure, viewed at a near edge-on orientation. The central bulge appears prominent, exhibiting a concentrated, yellowish-orange hue indicative of an older stellar population. The disk displays a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. Morphological analysis indicates a possibility of ongoing mergers or interactions given the slight disturbances and asymmetries observed within the disk and around the central bulge. The galaxy exhibits notable star formation, inferred from the blue color and the overall luminosity of the disk. The stellar mass of the galaxy appears substantial, based on its absolute magnitudes. The object is distant, confirmed by its measured redshift. The galaxy displays a faintness in the G band compared to the R and Z bands.
