The galaxy presents as a spiral type, with a relatively bright, centrally located bulge region. The spiral arms are well-defined, exhibiting a somewhat grand design structure. They appear continuous and extend outward from the central region, exhibiting a noticeable blueish tint, suggesting active star formation regions within them. The overall disk structure appears relatively flat when viewed from our vantage point, with no indications of significant edge-on morphology. Some irregularities are visible in the arm structure, hinting at possible gravitational interactions or minor disturbances. Overall, the galaxy appears relatively isolated within the field of view. The bulge is yellowish-white suggesting older star populations here.
