The galaxy appears as an elongated structure with a relatively smooth, centrally concentrated luminosity profile. Its overall shape is distinctly cigar-shaped, suggesting an elliptical morphology or a disk galaxy viewed edge-on. A faint bluish hue is observed in the main body, which may indicate the presence of younger stars.

There are two distinct regions of interest. The first is yellow and green in color. The second region is also yellow, and seems to have red and blue in it. These regions could indicate enhanced star formation or the presence of dust lanes, which could also potentially indicate minor disturbances. Further analysis is required to confirm these interpretations.
