The galaxy appears as a somewhat elongated, disk-like structure with a relatively smooth and concentrated central bulge. There's a slight asymmetry to the disk, hinting at possible minor disturbances, though a well defined spiral structure is not evident. The color profile suggests a predominantly older stellar population, exhibiting a reddish-yellow hue throughout the disk, which fades as it reaches the outer regions. There is evidence of bluer regions within the central area, suggestive of more recent star formation which is more concentrated toward the core. Overall, the galaxy seems to be an intermediate stage in its evolution, showing characteristics of both spiral and elliptical galaxies.
