The galaxy presents as an elliptical or lenticular type, characterized by a smooth, diffuse light distribution with an approximate half-light radius of around 10 kiloparsecs. Its color gradient indicates a primarily older stellar population, exhibiting a redder hue in comparison to spiral galaxies with active star formation. A secondary, smaller object is in close proximity, potentially representing a satellite galaxy or a background object undergoing a gravitational interaction with the main galaxy. The galaxy's morphology is mostly undisturbed, indicating a period of relative stability. Limited tidal features are visible, suggesting a low rate of ongoing or recent major mergers.
