The galaxy presents as a disk-shaped structure seen edge-on. The disk exhibits a moderately concentrated central bulge region, with an overall smooth appearance, lacking distinct spiral arm features. The color profile suggests a relatively evolved stellar population, transitioning from blue towards redder hues towards the core. There appears to be some asymmetry to the galaxy's disk, possibly indicating a minor gravitational interaction or internal dynamic disturbance.  The image is suggestive of a large galaxy, likely with a substantial stellar mass.
