The galaxy presents as a generally smooth object, with a slightly elliptical morphology. A bright, concentrated central bulge is observed, indicating a relatively high stellar density in the core. The color distribution exhibits a subtle gradient, with the central region appearing more yellowish, possibly indicative of an older stellar population, while the outer regions are more bluish, suggesting the presence of younger, hotter stars and potential ongoing star formation. There's a hint of asymmetry or a very subtle distortion in the outer disk. There is no clear spiral arm structure, and a slight disturbance in the structure suggests the possibility of a minor interaction with another galaxy. It is difficult to be certain about this based on the image. The roundness suggests that is is close to the edge of the galaxy. 
