The galaxy presents as a centrally concentrated, smooth elliptical type, exhibiting a high degree of radial symmetry. The core is a bright, almost uniform yellow-white, suggesting an older stellar population. Moving outward, the galaxy appears more diffuse, with a gradual decrease in surface brightness. There is a subtle color gradient, with the outer regions appearing slightly redder than the core. No distinct spiral arms, dust lanes, or other prominent features indicative of recent star formation are visible. Overall, the galaxy's morphology suggests a relatively evolved system, likely dominated by older stars and a low star formation rate. Any ongoing star formation appears to be limited and not significantly affecting the overall color or morphology.