This galaxy presents as an edge-on spiral, exhibiting a prominent, somewhat rounded central bulge that appears yellowish in color, suggesting an older stellar population. The disk is clearly visible as a flattened structure extending from the bulge, with a noticeable dust lane that bisects it. This obscuration indicates the presence of significant amounts of interstellar dust and gas within the disk. The disk appears somewhat disturbed, perhaps indicating a minor interaction. Overall, the galaxy shows properties consistent with a moderately massive system with ongoing, but potentially low, star formation activity.
