This galaxy presents as a spiral type, exhibiting a prominent disk structure with a central bulge. The spiral arms are clearly defined, displaying a tightly wound morphology. The color distribution suggests active star formation regions within the spiral arms, indicated by a bluer hue, contrasting with the yellower, older stellar populations concentrated within the bulge. There is evidence of some disturbance or possible interaction, as suggested by the slightly asymmetric arm structure. The bulge appears moderately sized. There is no clear evidence of a strong bar feature.
