This galaxy appears to be a relatively smooth, centrally concentrated object. The light profile suggests a significant bulge component, with a gradual decrease in surface brightness outward from the center. The central region exhibits a yellowish-white hue, potentially indicating an older stellar population and a lack of significant ongoing star formation. The outer regions of the galaxy show a bluer tinge in comparison, perhaps indicative of a younger stellar population. There is no obvious spiral structure or prominent dust lanes visible in the image. The overall morphology suggests that this galaxy may be an elliptical or lenticular galaxy, with a high probability of being an elliptical galaxy. There is no obvious evidence of a major ongoing merger or strong tidal interactions, however, there may be minor disturbances present. The galaxy appears relatively isolated in the field of view, suggesting it may be a field galaxy rather than a member of a dense cluster. The apparent roundness of the galaxy suggests that it is viewed close to face-on.
