The galaxy presents a predominantly blue hue, suggesting active star formation regions within its structure. It appears to be a spiral galaxy with a well-defined disk, though the angle of inclination makes it difficult to ascertain the exact morphology of the spiral arms. There seems to be two or more dominant arms.

The central bulge appears moderately prominent. There is no discernible evidence of a strong bar feature bisecting the nucleus.

The overall color profile indicates a population of younger, hotter stars alongside an older stellar population in the bulge, suggesting ongoing galactic evolution. There is possible evidence of tidal disturbances or minor mergers in the disk structure. These are difficult to discern without more detailed spectroscopic information.
