The galaxy presents as a spiral type with two prominent, well-defined spiral arms extending from a central bulge. These arms exhibit a moderate winding, neither tightly wound nor overly loose. The central bulge appears relatively large, though not entirely dominant, and displays a yellowish hue, potentially indicative of an older stellar population. The disk is observed face-on, revealing its spiral structure. There is no clear evidence of a strong bar structure, but a subtle linear feature could suggest a weak bar presence. The overall color profile suggests a mix of stellar populations, with bluer regions potentially indicating ongoing star formation within the spiral arms. There are no immediately apparent signs of significant merger activity or major tidal disturbances. The galaxy appears relatively undisturbed.
