The galaxy presents as an object with an ellipsoidal morphology. The light distribution appears relatively smooth and centrally concentrated. There's a noticeable color gradient with the core appearing yellower, potentially indicating an older stellar population or significant dust obscuration towards the center. The outer regions show bluer tints which may indicate younger star formation activity. The galaxy appears relatively isolated with no obvious signs of interaction with other galaxies or tidal features from previous interactions, though there is a small disturbance that suggests a minor merging event or tidal interaction. Overall, the structure of the galaxy suggests a potential transition between a spiral and elliptical structure with hints of past dynamical disturbances.
