The galaxy presents as an elongated, edge-on disk galaxy. A distinct central bulge is apparent, exhibiting a yellowish hue, indicating a population of older stars. The disk itself appears relatively smooth, with a subtle bluish tinge at the edges, possibly indicative of more recent star formation within the galactic plane. The overall form is consistent with a Sersic profile. The axial ratio suggests a highly flattened disk. There is no obvious evidence of strong spiral arm structure. The galaxy exhibits a relatively low star formation rate.