The galaxy presents as a relatively smooth, elliptical or lenticular structure. The central bulge is prominent and displays a concentrated, yellowish hue, suggestive of an older stellar population. Moving outwards from the core, the light gradually fades into a less defined halo. There are no visible spiral arms or distinct dust lanes present. The morphology appears largely undisturbed, with no clear signs of recent major mergers or interactions. The overall color indices lean towards the red end of the spectrum, possibly indicating a lower rate of star formation. The galaxy exhibits a roughly rounded shape.
