The galaxy appears to be a disk galaxy, viewed at a significant inclination. The central bulge is prominent and exhibits a yellowish-red hue, suggesting an older stellar population. The disk shows fainter, bluer regions, potentially indicating areas of recent or ongoing star formation. There is evidence of some subtle disturbances in the outer regions of the disk, perhaps due to a minor interaction or past merger event. The galaxy’s overall morphology seems to lean towards a relatively smooth structure, though some distinct features are visible.
