The galaxy presents as a relatively compact object with a dominant central bulge exhibiting a yellowish hue, suggesting an older stellar population concentrated towards the core. Fainter and more diffuse disk-like structures extend outwards from the central region. These outer regions appear slightly bluer in color, possibly indicating regions of more recent star formation. Some disturbances are present, it could be a minor interaction or tidal disturbance. Overall, it is likely a spiral galaxy seen at a moderate distance, with evidence of both older and younger stellar populations and possibly a small interaction.
