The galaxy presents as a somewhat face-on or moderately inclined spiral galaxy with a clearly defined central bulge. The bulge exhibits a yellowish hue, suggestive of an older stellar population. The disk component displays a bluer tint overall, indicative of ongoing star formation. The spiral arms are somewhat flocculent and not as tightly wound, showing hints of some irregularity. There is possible minor disturbance within the spiral arms, hinting at a minor interaction or internal dynamic process. The galaxy appears to be generally undisturbed in its overall morphology, with no strong evidence of a major merger event. The galaxy exhibits a relatively moderate star formation rate based on its color profile.
