The galaxy presents as a moderately luminous, disk-shaped structure, viewed at an inclined angle relative to our line of sight. The central bulge appears concentrated and bright, indicating a significant stellar population. The disk component exhibits a smooth texture, lacking prominent spiral arm structures. There are indications of some disturbances in the outer regions of the disk, suggesting possible interactions or minor mergers. The galaxy's color gradient transitions from a bluer hue in the outer disk to a slightly redder tone toward the central bulge, possibly indicating ongoing or recent star formation. The overall morphology appears to be somewhere between a smooth elliptical and a disturbed spiral.
