The galaxy presents a generally smooth morphology. It appears elongated, exhibiting a cigar-like shape, but with some deviation from a perfect ellipse. The color distribution is not uniform across the galaxy's body. A central concentration shows a distinctly bluer hue, indicative of potentially younger, hotter stellar populations. This region is surrounded by a more diffuse area that shows redder tones, possibly signifying the presence of older stars or dust obscuration.

There is evidence of a minor disturbance in the galaxy's structure. The overall structure appears to be somewhat irregular, suggesting possible gravitational interaction or recent merger activity. There may be subtle tidal features extending away from the main galactic body, though these are not sharply defined.
