The galaxy presents a smooth, elliptical appearance, with a concentrated central bulge. The light distribution suggests a lack of significant spiral arm structure, with the majority of light emanating from a relatively compact region. The galaxy exhibits a yellow-reddish hue throughout the body, indicating an older stellar population with minimal ongoing star formation. There are faint indications of a possible minor disturbance in the galaxy’s morphology, as one side has a slight asymmetry. This could be indicative of a past or ongoing minor merger event. Overall, the galaxy appears as a relatively massive, quiescent system with little evidence of recent star formation.
