The galaxy presents a distinct spiral morphology, exhibiting well-defined arms extending from a central bulge. These arms appear tightly wound, creating a sense of inward curvature. The color profile suggests ongoing star formation activity within the spiral arms, with a notable blue hue indicative of young, hot stars. The central bulge appears relatively prominent, exhibiting a moderate size in relation to the overall galactic disk. A faint bar-like structure may be present, though its definition is somewhat ambiguous. There is no obvious evidence of a major merger or significant tidal disturbances. Overall, the galaxy appears to be a well-formed spiral galaxy, showing characteristics of active star formation within its disk.