The galaxy presents an elongated morphology, appearing significantly longer than it is wide. The luminosity distribution is not uniform. There appears to be a central bulge exhibiting a yellowish-white hue, suggesting a population of older stars. Moving outwards along the major axis, there is a distinct color gradient shifting towards bluer tones, particularly noticeable at one end, which is a pale blue. At the end of the galaxy on the blue side, there is a pocket of green visible, which suggests intense star formation. This transition implies the presence of younger, hotter stellar populations in the outer regions. Overall, the structure lacks a clear spiral arm organization. A slight disturbance may be present on the edges of the object.
