The galaxy presents as a concentrated, centrally luminous object, displaying an overall smooth morphology. Its shape appears to be generally ellipsoidal, though not perfectly spherical. There is a hint of elongation along one axis, but this is not strongly pronounced. The galaxy's light distribution suggests a dominant bulge component with a relatively faint and indistinct disk. There's no clear evidence of spiral arms or other prominent features within the disk, though low resolution and distance could obscure such features.

The color profile indicates a redder hue, particularly toward the central region, suggestive of an older stellar population. There's a subtle gradient outwards, with a slightly bluer tint apparent in the outer regions. No significant dust lanes or patches of active star formation are immediately discernible from the image. There are no obvious signs of tidal disturbances or ongoing merger activity, though very faint features might be present at the limits of the image resolution and depth.
