This galaxy appears to be a relatively small, disk-shaped structure. Its morphology is not entirely smooth, indicating some level of internal structure. There is a central, brighter region, possibly indicating a galactic bulge or a higher concentration of stars. The color profile suggests a mix of stellar populations, with bluer hues concentrated in some regions. The edges of the disk appear somewhat disturbed or irregular. There appears to be possible merger activity, with signs of tidal disturbances or ongoing interactions with another galaxy. The overall shape exhibits a general disk morphology, but the irregularities and disturbances hint at a complex formation history or ongoing interactions. 
