The galaxy presents as a relatively smooth, disk-shaped structure viewed at an oblique angle. A central bulge region is apparent, exhibiting a brighter, more concentrated luminosity. The overall color profile suggests a mix of stellar populations, with a dominant blue-white hue in the disk and a slightly redder tone in some regions, possibly indicating areas of ongoing or recent star formation and older stellar populations, respectively. There is evidence of some disturbance or irregularity in the galaxy's form, although it is unclear from the image whether this is due to internal processes or interactions with neighboring galaxies. There may be slight tidal tails but not fully significant based on the low resolution of the image. Overall, the galaxy's morphology leans towards a disk galaxy with a moderate bulge and some signs of interaction or internal activity.
