The galaxy presents a moderately inclined disk structure. Evidence suggests the presence of spiral arms, though they appear somewhat faint and diffuse. A central bulge is visible, but does not dominate the overall structure. There is no obvious sign of a strong bar feature crossing the galaxy’s nucleus. The outer regions of the disk show irregularities that suggest possible interactions or disturbances, though no major merging event is immediately apparent. Star formation appears to be relatively low, correlating with the faint nature of the arms. The galaxy's color indicates that the galaxy contains a population of older stars.
