The galaxy appears to be an elliptical galaxy at a redshift of approximately 0.13, indicating a substantial distance. It presents a smooth, largely featureless morphology. The galaxy's shape is generally round, showing a high degree of rotational symmetry. There is no obvious evidence of spiral arms or a prominent disk structure. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer edges.

Based on its color indices, the galaxy exhibits a moderately red appearance, indicative of an older stellar population with a lower rate of ongoing star formation. There are no readily apparent signs of recent or significant merger activity, though minor disturbances cannot be ruled out.
