The galaxy presents as a relatively compact object with a smooth, elliptical morphology. It appears to be a spheroid-dominated system with little evidence of spiral arms or a prominent disk structure. The color gradient suggests a redder hue, potentially indicating an older stellar population and a lower rate of ongoing star formation. The galaxy's shape is elongated, exhibiting an intermediate aspect ratio between round and cigar-shaped. No major disturbances are visible in its structure, nor are there any obvious signs of an ongoing major merger event. There might be a very slight asymmetry to the light distribution, but the dominant impression is one of regularity. 
