This galaxy presents a generally smooth morphology, appearing elliptical in shape rather than exhibiting prominent spiral arms or a well-defined disk structure. There is a noticeable concentration of light towards the central region, indicating a bulge possibly dominated by older stellar populations. The outer regions of the galaxy appear more diffuse, gradually fading into the background sky. The galaxy exhibits a slight blue hue which may imply ongoing star formation. No significant tidal features or signs of a recent major merger event are apparent, although a minor disturbance or interaction cannot be ruled out based on this image alone. 
