This galaxy presents as a relatively smooth, elongated structure, possibly a disk galaxy viewed at an angle. The central bulge appears bright and concentrated, exhibiting a yellowish hue indicative of an older stellar population. The outer regions show a subtle flattening and a bluer color, suggesting the presence of younger stars and ongoing star formation, though at a seemingly modest rate. There is no prominent spiral arm structure discernible in the image, nor are there any obvious signs of a major merger event. Minor disturbances cannot be entirely ruled out. Overall, the galaxy seems to be in a relatively quiescent state.
