The galaxy presents as a somewhat elongated, cigar-shaped structure with a predominantly smooth light distribution. A slight color gradient is observed along its major axis, transitioning from a bluer hue at one end to a redder hue at the other. This color difference hints at variations in stellar populations or dust content. The overall smoothness suggests that it is likely an elliptical galaxy that may be in the process of merging. The estimated size and shape are consistent with an elliptical galaxy. Despite the general smoothness, closer inspection reveals a subtle hint of possible disturbances within the galaxy's morphology, such as asymmetric features which may indicate a minor interaction with another galaxy. A significant portion of the galaxy appears to be composed of older stellar populations, yet there is an indication of ongoing star formation activity. The galaxy does not exhibit a prominent disk-like structure.
