The galaxy presents as an elliptical morphology, with a smooth, centrally concentrated light distribution. The color profile indicates a relatively evolved stellar population, displaying a yellow-orange hue characteristic of older stars. There is a lack of discernible spiral arm structure or distinct dust lanes, suggesting it is not a spiral galaxy.

The shape appears to be somewhat elongated rather than perfectly spherical. There might be evidence of minor tidal interactions, but overall, the galaxy seems relatively undisturbed. The limited evidence of active star formation suggests a passively evolving system. The object has an estimated diameter of approximately 6 kpc based on its redshift, and the absence of blue light implies limited current star formation.
