The galaxy presents an elongated, somewhat cigar-shaped morphology. The light distribution appears relatively smooth, with a subtle central concentration. There is a hint of internal structure, possibly a faint disk or spiral arms, though the resolution is insufficient to confirm. The galaxy's color profile suggests a mix of stellar populations. The central region exhibits a slightly redder hue, potentially indicating an older stellar population or dust obscuration, while the outer regions display a bluer color, possibly due to more recent star formation. Overall, the galaxy appears relatively undisturbed, lacking significant signs of ongoing mergers or tidal interactions, however, there are slight disturbances that could indicate a minor merger.
