The galaxy presents as an elongated structure, suggestive of an edge-on or highly inclined disk galaxy. The central region exhibits a concentrated, bright core, indicative of a bulge component. The light distribution gradually fades from the core outwards, displaying a smooth profile. There is a hint of dust lane obscuration along the major axis, potentially bisecting the galaxy. The outer disk appears relatively faint. Possible asymmetries or disturbances may be present in the disk. The galaxy shows redder colors, possibly indicating a population of older stars.
