The galaxy exhibits a clear disk morphology, viewed at a slight angle from edge-on. Prominent spiral arm structures are visible but somewhat diffuse, without sharp definition. A central bulge is noticeable, appearing moderately sized and brightly illuminated. The overall color distribution indicates a mix of stellar populations, with the central region appearing yellower and the outer regions showing hints of bluer hues, potentially indicating regions of more recent star formation. There appears to be some minor disturbance in the galaxy's structure, possibly suggestive of tidal interactions or a minor merger event in its recent history. A faint bar structure may be present but is not clearly defined.
