The galaxy presents as a spiral type, though with some notable inclination relative to our line of sight. The spiral arms are apparent, exhibiting a somewhat flocculent morphology, and appear moderately tightly wound. There is evidence of ongoing star formation within the arms, indicated by the bluer hues. A prominent bulge is observed, characterized by a more yellow/red hue indicative of an older stellar population. The bulge appears to be of moderate size, not dominating the overall galactic structure. There is a suggestion of a bar-like structure, but it is not particularly pronounced. There does not appear to be any major interaction with other galaxies or strong evidence of a recent merger, though there is some irregularity within the disk structure which may indicate minor disturbance. Overall, the galaxy shows characteristics of a relatively massive system with a moderate rate of star formation, and an evolved bulge component.
