The galaxy presents as an elongated system, appearing cigar-shaped. The light distribution suggests a central bulge, possibly obscured, with extensions indicative of a disk structure, though not clearly defined. There is a noticeable asymmetry in the light distribution, hinting at possible interactions or tidal disturbances. The color gradient transitions from bluer hues in the outer regions, potentially indicating younger stellar populations associated with star formation, to redder colors towards the core.

The overall structure does not appear smooth; rather, it has a somewhat disrupted appearance, suggesting a non-negligible star formation rate and potentially some morphological disturbance. This could be due to a recent or ongoing merger event, or perhaps some internal instability within the galactic disk.
