The galaxy presents as a spiral type, exhibiting distinct features suggesting active star formation. A prominent, albeit somewhat obscured, central bulge is visible, surrounded by a disk structure. The spiral arms are well-defined and appear tightly wound. A bright, elongated feature is seen, possibly an edge-on disk galaxy merging with the spiral galaxy. The overall color profile indicates a mixed stellar population, with bluer regions concentrated in the arms, indicative of younger stars and ongoing star formation, and a redder hue in the central bulge suggesting an older stellar population. The galaxy shows some signs of gravitational interaction, possibly due to the presence of the smaller edge-on galaxy.
