The observed galaxy appears to be a relatively compact object. Its overall morphology indicates it possesses a smooth, somewhat amorphous structure lacking a clearly defined spiral arm or bar feature. There is some asymmetry in the galaxy’s light distribution, indicating possible interactions with other objects or recent disturbance. The color gradient suggests that the galaxy is composed of older stellar populations with a redder color profile. There is a suggestion of a faint tidal feature extending from the galaxy suggesting minor interactions or disturbances in its recent past. The core of the galaxy is not well defined, which suggests a relatively low central concentration of light. It appears to be a lower luminosity object. Overall, the galaxy exhibits characteristics consistent with an elliptical galaxy that has undergone some gravitational interactions.
