The galaxy presents a discernible disk structure, viewed at an angle that indicates it is not edge-on. The morphology is dominated by spiral arms. These arms appear to have a relatively tight winding, originating from a central bulge. The bulge appears to be of moderate size relative to the disk. The galactic center is a bright, concentrated region, possibly indicating the presence of a supermassive black hole and/or a high density of stars. The color distribution suggests a mix of stellar populations within the galaxy. The central region exhibits a yellowish hue, which may indicate an older stellar population. The spiral arms display a bluer color, potentially indicating ongoing star formation. The overall structure does not show significant signs of major interaction or merging events, although some minor disturbances or asymmetries may be present.
