The galaxy appears to be a spiral type with a moderately inclined disk. There's evidence of some disturbance in the morphology, potentially indicating a minor interaction or merger. The central bulge is relatively bright and concentrated, with a yellowish-white hue. The spiral arms are not very well defined, appearing somewhat flocculent and patchy in their structure. The galaxy exhibits a range of colors across its structure, with bluer regions possibly associated with star formation in the spiral arms and redder regions likely associated with older stellar populations, particularly in the bulge. Overall, the galaxy's morphology suggests it is undergoing or has recently undergone some form of interaction that has disrupted its regular spiral structure.
