The galaxy presents as a spiral type, viewed at a moderate angle relative to its disk. Its morphology suggests a classification between Sa and Sb. The spiral arms are tightly wound and display a flocculent structure, appearing less defined and patchy rather than grand design. Multiple arms are discernible. A central bulge is present, exhibiting moderate size. The bulge appears relatively smooth and concentrated, suggesting an older stellar population. There is no obvious bar structure visually apparent. The overall color profile indicates a mix of stellar populations, with bluer hues in the spiral arms likely indicating regions of active star formation, while the yellowish central bulge possibly houses older, redder stars. No significant signs of ongoing major merging events are observed, although some minor asymmetry could indicate past interactions or minor disturbances. The galaxy appears reasonably well-defined, suggesting a relatively isolated system or one where any tidal interactions are currently minimal.
