The galaxy presents as a relatively smooth object with a moderate ellipticity. The light distribution suggests a central bulge, likely composed of older stellar populations given its yellowish-orange hue. The overall structure implies a disk component, but the disk lacks distinct spiral arms or prominent dust lanes; it appears relatively featureless. The galaxy's color profile indicates a higher concentration of redder stars towards the center, and a subtle bluer trend towards the outer edges. There is some potential minor asymmetry in the galaxy’s outer regions, but this is not particularly pronounced. Based on color and morphology, it is likely a disk galaxy dominated by older stellar populations with a moderate size.
