The galaxy presents as a spiral type, viewed at an oblique angle relative to our line of sight. Evident spiral arm structures emanate from the central region. These arms are discernible but somewhat flocculent in appearance, displaying patchy distributions of star formation regions, suggested by the presence of bluer hues along the arms. The central bulge appears moderately sized and exhibits a smoother, more uniform color profile, indicative of an older stellar population. The overall color of the galaxy suggests ongoing star formation, although the specific star formation rate seems relatively low. No significant tidal distortions or indications of a major merger event are readily apparent, although there might be some minor disturbances within the disk. There may be some slight evidence of a weak bar structure. The galaxy disk extends noticeably beyond the bulge, with the arms gradually fading into the background. The overall morphology indicates a relatively undisturbed spiral galaxy, with a mix of old and young stellar populations distributed throughout its structure.