The galaxy presents as a largely homogenous, smooth structure, lacking prominent spiral arms or a distinct bar. The central region exhibits a higher surface brightness and a yellowish hue, suggesting an older stellar population is dominant in the core. The galaxy's overall shape is close to circular, indicating it's likely an elliptical or S0 type galaxy. Fainter, diffuse light extends outwards from the core, gradually fading into the background sky. There is a very slight asymmetry to the galaxy's outer isophotes, but it does not suggest any major ongoing merger event. There is no evidence of significant dust lanes or prominent star formation regions visible within the galaxy itself based on the image. 
