The galaxy presents as a relatively smooth, elliptical morphology. The core region appears as a concentrated area of high luminosity, exhibiting a slightly reddish hue. Moving outward from the core, the galaxy transitions to a bluer color. The overall shape is moderately elongated, somewhere between round and cigar-shaped, displaying a near uniform luminosity gradient moving from the center to the outer edges. There is no strong evidence of significant spiral arm structure, tidal disturbances, or an active galactic nucleus based on the image data. This suggests it may be an older galaxy with a moderate rate of star formation. 
