The galaxy appears as a relatively smooth and centrally concentrated object, exhibiting a nearly circular morphology. There is little evidence of significant spiral arm structure or irregular features. The color profile suggests a higher concentration of older stellar populations, as indicated by the redder hue. There might be a slight hint of a central bulge, further supporting the presence of an evolved stellar population. There appear to be no mergers occurring with neighboring galaxies or obvious signs of disturbance of the internal structure.
