The galaxy presents a predominantly smooth morphology, with a high degree of central concentration. The core exhibits a bright, relatively well-defined nucleus, surrounded by a more diffuse halo. The overall shape appears close to circular, lacking any pronounced elongation or asymmetry. There is evidence of a potential interaction or tidal disturbance in the lower part of the galaxy, with what appears to be a secondary object or distorted spiral arm feature, possibly indicating a minor merger or ongoing gravitational interaction. There is a faint reddish hue and a hint of bluer light, which may indicate regions of lower level star formation. The galaxy appears relatively undisturbed overall, with a dominant smooth component and a subtle indication of recent or ongoing interaction.
