The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, with a bright, yellowish core gradually fading into a more diffuse outer region. The core exhibits a relatively homogenous color, suggesting an older stellar population. There is a subtle color gradient moving outwards, with the outer regions exhibiting a slightly bluer hue, potentially indicative of a younger stellar population or a lower metallicity. No distinct spiral arms or prominent dust lanes are visible. There is a faint indication of some slight disturbance within the galaxy, which could imply past minor interactions. The object appears largely undisturbed with no clear signs of tidal tails or significant morphological distortions.
