The galaxy presents a relatively smooth morphology, appearing as a somewhat rounded, yet not perfectly circular, distribution of light. There is no strong evidence of spiral arm structure or a prominent central bulge. The galaxy exhibits a color gradient, appearing redder in its central regions, which may indicate an older stellar population in the core. Moving outwards, the color shifts towards a slightly bluer hue, potentially suggesting the presence of younger, hotter stars within the galaxy's outer regions, perhaps due to ongoing or recent star formation. The overall structure seems undisturbed, with no clear signs of major mergers or tidal distortions. The galaxy's light is somewhat diffuse, lacking a sharp, well-defined edge, characteristic of certain elliptical galaxies.
