The galaxy presents as a concentrated, elliptical morphology. The core region exhibits a significantly higher luminosity than the surrounding area, indicating a dense stellar population. There is a noticeable radial color gradient, with the core appearing more yellowish-white, suggesting an older stellar population compared to the outer regions. The outer regions show hints of blueish color, indicating some amount of star formation. The galaxy exhibits an overall smooth texture. Some slight asymmetry can be observed, indicating the possibility of past or ongoing minor interactions. 
