The galaxy presents a predominantly smooth morphology, exhibiting a centrally concentrated light profile. The core region appears to have a yellow-reddish hue, suggesting an older stellar population. The galaxy's shape is generally elliptical, showing slight deviations from a perfect circle. There is no discernible spiral arm structure or a prominent disk component. Overall, the galaxy's structure indicates that it is relatively undisturbed, without any evidence of ongoing major mergers or significant tidal interactions.
