The galaxy presents as a moderately inclined, disk-shaped system. The central bulge is not prominently defined but appears as a general concentration of light. The galaxy exhibits a dominant blue hue, particularly in the central region and along the apparent major axis, suggesting ongoing star formation.  The arms are not well-defined, but are not completely absent. The galaxy appears relatively smooth, with no clear evidence of major mergers or significant tidal disturbances, though possible minor disturbances are not ruled out. There is only some evidence of redder light, possibly signifying older stellar populations, towards the periphery of the disk. The overall morphology suggests an intermediate classification between a spiral and a lenticular galaxy.
