The galaxy presents as a spiral galaxy with a well-defined disk structure oriented at an angle to the line of sight, but not fully edge-on. Two main spiral arms are clearly visible, emanating from a central bar feature. The bar appears to be significant in size and brightness. The spiral arms exhibit a moderate winding pattern, neither tightly wound nor loosely extended. A central bulge is present, appearing smaller in size relative to the disk component. The overall color profile suggests active star formation. The spiral arms display a bluer hue, possibly indicative of younger stellar populations and ongoing star formation, while the central region shows a more yellow/orange tone, potentially suggesting an older stellar population. There appears to be no evidence of significant tidal disturbances or interactions with other galaxies.
