The galaxy presents as a spiral type, characterized by a prominent, moderately sized central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Two tightly wound spiral arms emerge from the central bulge, displaying a somewhat clumpy morphology. These arms are bluer in color, indicative of ongoing star formation regions. The overall disk appears relatively undisturbed, though there is some asymmetry in the arm structure, possibly due to minor gravitational interactions. There is evidence of a weak bar structure in the central region. The galaxy's angular size suggests it is a large galaxy, likely a massive spiral. The red shift indicates that it is at an intermediate distance.