The galaxy presents a largely smooth and centrally concentrated morphology. It appears elliptical in shape, being noticeably elongated along one axis and showing a high degree of radial symmetry. The core exhibits a bright, yellowish hue, suggesting an older stellar population dominating the central region. The color gradually transitions outwards, with fainter, bluer tones observed in the outer regions. There is no distinct dust lane or spiral arm structure visible, and based on visual inspection, the galaxy does not seem to be undergoing any major merging activity. There may be a very subtle disturbance in the form of a slight asymmetry in the galaxy's outer regions. 
