The galaxy presents as a highly elongated structure, suggesting it is likely an edge-on spiral or a lenticular galaxy. It exhibits a distinct central bulge with a yellowish hue, indicating a population of older stars. A fainter, bluer extended disk is visible, possibly indicative of ongoing star formation. The galaxy's smooth appearance suggests a relatively evolved system, potentially past its peak star-forming epoch, but with some residual activity. The overall morphology does not reveal any major disturbances or signs of ongoing mergers.
