The galaxy presents as a spiral with a discernible disk, viewed at a moderately inclined angle to our line of sight. It exhibits a noticeable central bulge that appears bright and yellowish. This suggests the presence of an older stellar population concentrated towards the center. The disk shows evidence of spiral arm structure, though it is somewhat flocculent and lacks the distinct, tightly wound arms often seen in grand design spirals. The color distribution across the disk indicates a mix of stellar populations, with bluer regions possibly indicating areas of active star formation, especially towards the outer edges of the disk. The galaxy does not appear to be undergoing a major merger or significant interaction with another galaxy, although there might be a minor disturbance or asymmetry in the disk structure. Based on this we can guess this galaxy has a stellar mass of approximately 10^11 solar masses, with a moderate amount of ongoing star formation.
