The galaxy presents as a concentrated central bulge surrounded by a less defined, somewhat asymmetrical disk. The central bulge appears to be primarily composed of older stellar populations, indicated by its reddish-orange hue. The outer regions of the disk show hints of bluer light, suggesting the presence of younger, hotter stars and potentially ongoing star formation, although this is not readily apparent in this particular image. The overall structure shows some signs of disturbance or interaction, but the disturbance does not appear to be significantly disrupting the shape of the galaxy. The edges of the disk are fairly smooth, and the galaxy appears to be relatively isolated.
