The galaxy presents as an elongated, disk-shaped structure, viewed at a high inclination. The central bulge exhibits a yellowish-orange hue, suggesting an older stellar population. Fainter spiral arms are visible extending from the central region, appearing somewhat diffuse. The outer regions of the disk show a bluer tint, potentially indicating regions of more recent star formation. There is some evidence of minor tidal disturbance or interaction with a possible companion galaxy located near it. Overall, this galaxy appears to be a massive disk galaxy with ongoing, but potentially diminishing, star formation. The smooth morphology suggests an evolved system, but the minor irregularities hint at a complex formation history.
