The galaxy exhibits a morphology consistent with a spiral type. The galaxy displays a prominent central bulge, appearing moderately sized in relation to the overall disk. Faint spiral arm structures are visible, although they are not highly defined. There is no strong indication of a central bar feature. The galaxy's color profile suggests a mix of stellar populations, with a yellowish hue concentrated in the bulge region, potentially indicating older stars. Some bluer areas can be seen within the spiral arms, which may indicate regions of recent or ongoing star formation. The disk appears slightly inclined with respect to our line of sight, and there may be some level of minor disturbance or interaction affecting the overall structure of the galaxy, but it is not obvious. The galaxy exhibits a moderate size. 
